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'Intrusioni' immagini e video risultati page 1 of 1

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Immagini di 'Intrusioni' trovate, 50

Black cabasa with tan
 
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Black cabasa with tan

Stock, Chris

SKC3883682

Black cabasa with tan

Stock, Chris

SKC3883682

Girl with Cat, 1943 (oil on canvas)
 
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Copyright/Diritti d'Autore
  • In Copyright
Girl with Cat, 1943 (oil on canvas)

Citti Ferreira, Lucy (1911-2008)

TLH496340

Girl with Cat, 1943 (oil on canvas)

Citti Ferreira, Lucy (1911-2008)

TLH496340

Double chanter and cowhorns on a set of Arabic bagpipes
 
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  • Content within this photograph may require additional clearances (eg: trademark and personality rights) depending on Licensee's specific use of material, which may include book and magazine cover use.
Double chanter and cowhorns on a set of Arabic bagpipes

Stock, Chris

SKC3837319

Double chanter and cowhorns on a set of Arabic bagpipes

Stock, Chris

SKC3837319

Double chanter and cowhorns on a set of Arabic bagpipes
 
Restrizioni immagine
  • Content within this photograph may require additional clearances (eg: trademark and personality rights) depending on Licensee's specific use of material, which may include book and magazine cover use.
Double chanter and cowhorns on a set of Arabic bagpipes

Stock, Chris

SKC3837321

Double chanter and cowhorns on a set of Arabic bagpipes

Stock, Chris

SKC3837321

Indian singer and sarangi player
 
Indian singer and sarangi player

Noel, Odile

ODN3853653

Indian singer and sarangi player

Noel, Odile

ODN3853653

Indian singer and sarangi player
 
Indian singer and sarangi player

Noel, Odile

ODN3853655

Indian singer and sarangi player

Noel, Odile

ODN3853655

Double chanter and cowhorns on a set of Arabic bagpipes
 
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Double chanter and cowhorns on a set of Arabic bagpipes

Stock, Chris

SKC3837324

Double chanter and cowhorns on a set of Arabic bagpipes

Stock, Chris

SKC3837324

Double chanter and cowhorns on a set of Arabic bagpipes
 
Restrizioni immagine
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Double chanter and cowhorns on a set of Arabic bagpipes

Stock, Chris

SKC3837322

Double chanter and cowhorns on a set of Arabic bagpipes

Stock, Chris

SKC3837322

AFGHANS STAGE PROTEST OVER ALLEGED BORDER INTRUSIONS IN KABUL, 2003-07-07 (photo)
 
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AFGHANS STAGE PROTEST OVER ALLEGED BORDER INTRUSIONS IN KABUL, 2003-07-07 (photo)

Ahmad Masood

REU7829357

AFGHANS STAGE PROTEST OVER ALLEGED BORDER INTRUSIONS IN KABUL, 2003-07-07 (photo)

Ahmad Masood

REU7829357

Indian singer and sarangi player
 
Indian singer and sarangi player

Noel, Odile

ODN3853654

Indian singer and sarangi player

Noel, Odile

ODN3853654

Trompete / trumpet -
 
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Trompete / trumpet -

Stock, Chris

SKC3888031

Trompete / trumpet -

Stock, Chris

SKC3888031

Advertisement for Riccardi pianos, 1928 (lithograph)
 
Advertisement for Riccardi pianos, 1928 (lithograph)

XLF3781775

Advertisement for Riccardi pianos, 1928 (lithograph)

XLF3781775

Triptych depicting the Coronation of the Virgin (left panel: saints, angel musicians and the kneeling Cardinal) (tempera on panel)
 
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Triptych depicting the Coronation of the Virgin (left panel: saints, angel musicians and the kneeling Cardinal) (tempera on panel)

Angelico, Fra (c.1387-1455) & Lippi, F (c.1406-69)

XIR897839

Triptych depicting the Coronation of the Virgin (left panel: saints, angel musicians and the kneeling Cardinal) (tempera on panel)

Angelico, Fra (c.1387-1455) & Lippi, F (c.1406-69)

XIR897839

Art Themen - portrait
 
Art Themen - portrait

Noel, Odile

ODN3891399

Art Themen - portrait

Noel, Odile

ODN3891399

Art Themen - portrait
 
Art Themen - portrait

Noel, Odile

ODN3891428

Art Themen - portrait

Noel, Odile

ODN3891428

Illinois Jacquet - portrait
 
Illinois Jacquet - portrait

Noel, Odile

ODN3891431

Illinois Jacquet - portrait

Noel, Odile

ODN3891431

Salesperson Saeri Yokota at Matsushita Electric Co. in Tokyo demonstrates standard model Home Controller, equipped with a small computer to switch appliances on and off; the computer also warns of fires, intruders, gas leaks, bath temperature, etc, 1985-04-01 (photo)
 
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  • Content within this photograph may require additional clearances (eg: trademark and personality rights) depending on Licensee's specific use of material, which may include book and magazine cover use.
Il Content Partner applica le seguenti restrizioni
  • Minimum fee applies to this image;Only available to clients invoiced in Australia, Belgium, Brazil, Bulgaria, Canada, China, Cyprus, Czech Republic, Estonia, Finland, France, French Southern Territories, Greece, Hong Kong, Hungary, India, Ireland, Israel, Italy, Lebanon, Luxembourg, Mexico, the Netherlands, New Zealand, Portugal, Qatar, Republic of Korea, Romania, Russian Federation, Singapore, South Africa, Spain, Sweden, Switzerland, Taiwan, Turkey, United Arab Emirates, United Kingdom and United States
Salesperson Saeri Yokota at Matsushita Electric Co. in Tokyo demonstrates standard model Home Controller, equipped with a small computer to switch appliances on and off; the computer also warns of fires, intruders, gas leaks, bath temperature, etc, 1985-04-01 (photo)

Hatano, Masaharu

REU12029060

Salesperson Saeri Yokota at Matsushita Electric Co. in Tokyo demonstrates standard model Home Controller, equipped with a small computer to switch appliances on and off; the computer also warns of fires, intruders, gas leaks, bath temperature, etc, 1985-04-01 (photo)

Hatano, Masaharu

REU12029060

Gerry Mulligan - portrait
 
Gerry Mulligan - portrait

Noel, Odile

ODN3891424

Gerry Mulligan - portrait

Noel, Odile

ODN3891424

Gerry Mulligan - portrait
 
Gerry Mulligan - portrait

Noel, Odile

ODN3891425

Gerry Mulligan - portrait

Noel, Odile

ODN3891425

Gerry Mulligan - portrait
 
Gerry Mulligan - portrait

Noel, Odile

ODN3891423

Gerry Mulligan - portrait

Noel, Odile

ODN3891423

Illinois Jacquet - portrait
 
Illinois Jacquet - portrait

Noel, Odile

ODN3891446

Illinois Jacquet - portrait

Noel, Odile

ODN3891446

Dexter Gordon - portrait
 
Dexter Gordon - portrait

Noel, Odile

ODN3891409

Dexter Gordon - portrait

Noel, Odile

ODN3891409

Dexter Gordon - portrait
 
Dexter Gordon - portrait

Noel, Odile

ODN3891400

Dexter Gordon - portrait

Noel, Odile

ODN3891400

Crotales, orchestral percussion
 
Crotales, orchestral percussion

Graham Salter

SLR3829381

Crotales, orchestral percussion

Graham Salter

SLR3829381

Crotales, gongs and cymbals,
 
Crotales, gongs and cymbals,

Graham Salter

SLR3829584

Crotales, gongs and cymbals,

Graham Salter

SLR3829584

Roches Tuiliere et Sanadoire - Puy - de - Dome - Roche Tuiliere and Roche Sanadoire - Puy - de - Dome - These two rock pitons are magmatic intrusions that have cooled inside a volcanic cone. La Roche Sanadoire (right) was formed 2.2 million years ago. Roche Tuiliere is dated 1.9 million years. Roche Tuiliere (1288 m) and Roche Sanadoire (1286 m) dominate the Vallee du Chausse (glacial valley). Peaks of Roche Tuiliere and Roche Sanadoire, remnants of volcanic plugs (crater pipes) scoured out by an ancient glacier. Puy - de - Dome, Auvergne, France
 
Roches Tuiliere et Sanadoire - Puy - de - Dome - Roche Tuiliere and Roche Sanadoire - Puy - de - Dome - These two rock pitons are magmatic intrusions that have cooled inside a volcanic cone. La Roche Sanadoire (right) was formed 2.2 million years ago. Roche Tuiliere is dated 1.9 million years. Roche Tuiliere (1288 m) and Roche Sanadoire (1286 m) dominate the Vallee du Chausse (glacial valley). Peaks of Roche Tuiliere and Roche Sanadoire, remnants of volcanic plugs (crater pipes) scoured out by an ancient glacier. Puy - de - Dome, Auvergne, France

Sebastien Beaucourt

PIX4668843

Roches Tuiliere et Sanadoire - Puy - de - Dome - Roche Tuiliere and Roche Sanadoire - Puy - de - Dome - These two rock pitons are magmatic intrusions that have cooled inside a volcanic cone. La Roche Sanadoire (right) was formed 2.2 million years ago. Roche Tuiliere is dated 1.9 million years. Roche Tuiliere (1288 m) and Roche Sanadoire (1286 m) dominate the Vallee du Chausse (glacial valley). Peaks of Roche Tuiliere and Roche Sanadoire, remnants of volcanic plugs (crater pipes) scoured out by an ancient glacier. Puy - de - Dome, Auvergne, France

Sebastien Beaucourt

PIX4668843

Municipal Museum of the Sea
 
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Municipal Museum of the Sea

ELC849172

Municipal Museum of the Sea

ELC849172

ELLEN LEVIN AT HOUSE HEARING ON PERSONAL INTRUSION, 1998-05-21 (photo)
 
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ELLEN LEVIN AT HOUSE HEARING ON PERSONAL INTRUSION, 1998-05-21 (photo)

Larry Downing

REU7968410

ELLEN LEVIN AT HOUSE HEARING ON PERSONAL INTRUSION, 1998-05-21 (photo)

Larry Downing

REU7968410

AN AFGHAN MAN SHOUTS SLOGAN DURING A DEMONSTRATION IN KABUL, 2003-07-15 (photo)
 
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AN AFGHAN MAN SHOUTS SLOGAN DURING A DEMONSTRATION IN KABUL, 2003-07-15 (photo)

Ahmad Masood

REU7854932

AN AFGHAN MAN SHOUTS SLOGAN DURING A DEMONSTRATION IN KABUL, 2003-07-15 (photo)

Ahmad Masood

REU7854932

AFGHAN WOMEN RALLY DURING A DEMONSTRATION IN DOWNTOWN KABUL, 2003-07-15 (photo)
 
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AFGHAN WOMEN RALLY DURING A DEMONSTRATION IN DOWNTOWN KABUL, 2003-07-15 (photo)

Ahmad Masood

REU7915839

AFGHAN WOMEN RALLY DURING A DEMONSTRATION IN DOWNTOWN KABUL, 2003-07-15 (photo)

Ahmad Masood

REU7915839

South Korean opposition leader Lee Hoi-chang of the the Grand National Party delivers a special stat.., 2001 (photo)
 
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South Korean opposition leader Lee Hoi-chang of the the Grand National Party delivers a special stat.., 2001 (photo)

Yun Suk Bong

REU7467843

South Korean opposition leader Lee Hoi-chang of the the Grand National Party delivers a special stat.., 2001 (photo)

Yun Suk Bong

REU7467843

Eagle Nebula (IC 4703) and M16 star cluster in the Snake - The Eagle nebula in Serpens - The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 7000 light years distant
 
Eagle Nebula (IC 4703) and M16 star cluster in the Snake - The Eagle nebula in Serpens - The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 7000 light years distant

R. Gendler

PIX4620019

Eagle Nebula (IC 4703) and M16 star cluster in the Snake - The Eagle nebula in Serpens - The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 7000 light years distant

R. Gendler

PIX4620019

Eagle Nebula (IC 4703) and M16 star cluster in the Snake - Eagle nebula in Serpens - The Eagle Nebula is a cluster of massive young stars (M16) surrounded by clouds of gas and dust. The three columns in the center of the image were sculpted by the intense radiation emitted by these massive stars. Stars will be born in these clouds if they survive the intense radiation that erodes these pillars. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 6000 - 7000 light years distant
 
Eagle Nebula (IC 4703) and M16 star cluster in the Snake - Eagle nebula in Serpens - The Eagle Nebula is a cluster of massive young stars (M16) surrounded by clouds of gas and dust. The three columns in the center of the image were sculpted by the intense radiation emitted by these massive stars. Stars will be born in these clouds if they survive the intense radiation that erodes these pillars. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associ

PIX4620028

Eagle Nebula (IC 4703) and M16 star cluster in the Snake - Eagle nebula in Serpens - The Eagle Nebula is a cluster of massive young stars (M16) surrounded by clouds of gas and dust. The three columns in the center of the image were sculpted by the intense radiation emitted by these massive stars. Stars will be born in these clouds if they survive the intense radiation that erodes these pillars. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associ

PIX4620028

Eagle Nebula (IC 4703) and M16 star cluster in the Snake - Eagle nebula in Serpens - The Eagle Nebula is a cluster of massive young stars (M16) surrounded by clouds of gas and dust. The three columns in the center of the image were sculpted by the intense radiation emitted by these massive stars. Stars will be born in these clouds if they survive the intense radiation that erodes these pillars. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 6000 - 7000 light years distant
 
Eagle Nebula (IC 4703) and M16 star cluster in the Snake - Eagle nebula in Serpens - The Eagle Nebula is a cluster of massive young stars (M16) surrounded by clouds of gas and dust. The three columns in the center of the image were sculpted by the intense radiation emitted by these massive stars. Stars will be born in these clouds if they survive the intense radiation that erodes these pillars. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associ

PIX4619956

Eagle Nebula (IC 4703) and M16 star cluster in the Snake - Eagle nebula in Serpens - The Eagle Nebula is a cluster of massive young stars (M16) surrounded by clouds of gas and dust. The three columns in the center of the image were sculpted by the intense radiation emitted by these massive stars. Stars will be born in these clouds if they survive the intense radiation that erodes these pillars. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associ

PIX4619956

A GROUP OF AFGHANS STAGE A PROTEST IN KABUL, 2003-07-07 (photo)
 
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A GROUP OF AFGHANS STAGE A PROTEST IN KABUL, 2003-07-07 (photo)

Ahmad Masood

REU7880182

A GROUP OF AFGHANS STAGE A PROTEST IN KABUL, 2003-07-07 (photo)

Ahmad Masood

REU7880182

Eagle Nebula (IC 4703) and M16 star cluster in Snake - The Eagle nebula in Serpens - Eagle Nebula (IC 4703) and M16 star cluster in Snake. The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Image obtained with a telescope 61 cm in diameter. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 7000 light years distant. Image taken with a 24 - inch telescope
 
Eagle Nebula (IC 4703) and M16 star cluster in Snake - The Eagle nebula in Serpens - Eagle Nebula (IC 4703) and M16 star cluster in Snake. The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Image obtained with a telescope 61 cm in diameter. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are

Adam Block

PIX4620009

Eagle Nebula (IC 4703) and M16 star cluster in Snake - The Eagle nebula in Serpens - Eagle Nebula (IC 4703) and M16 star cluster in Snake. The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Image obtained with a telescope 61 cm in diameter. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are

Adam Block

PIX4620009

Eagle Nebula (IC 4703) and M16 star cluster in the Snake - M16, The Eagle Nebula in Serpens - The M16 star cluster is a cluster of young stars from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Image obtained by combining light through 3 different filters that highlight oxygen, hydrogen, and sulfur. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 7000 light years distant. Issue - line image presented here in false color
 
Eagle Nebula (IC 4703) and M16 star cluster in the Snake - M16, The Eagle Nebula in Serpens - The M16 star cluster is a cluster of young stars from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Image obtained by combining light through 3 different filters that highlight oxygen, hydrogen, and sulfur. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and a

PIX4620021

Eagle Nebula (IC 4703) and M16 star cluster in the Snake - M16, The Eagle Nebula in Serpens - The M16 star cluster is a cluster of young stars from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Image obtained by combining light through 3 different filters that highlight oxygen, hydrogen, and sulfur. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and a

PIX4620021

CROWDS LINE UP OUTSIDE THE BRITISH CONSULATE IN HONG KONG WAITING TO SIGN CONDOLENCE BOOK, 1997-09-02 (photo)
 
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CROWDS LINE UP OUTSIDE THE BRITISH CONSULATE IN HONG KONG WAITING TO SIGN CONDOLENCE BOOK, 1997-09-02 (photo)

Larry Chan

REU7936203

CROWDS LINE UP OUTSIDE THE BRITISH CONSULATE IN HONG KONG WAITING TO SIGN CONDOLENCE BOOK, 1997-09-02 (photo)

Larry Chan

REU7936203

AFGHAN POLICE CLEAR THE ROAD NEAR PAKISTANI EMBASSY IN KABUL, 2003-07-08 (photo)
 
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AFGHAN POLICE CLEAR THE ROAD NEAR PAKISTANI EMBASSY IN KABUL, 2003-07-08 (photo)

Ahmad Masood

REU7791448

AFGHAN POLICE CLEAR THE ROAD NEAR PAKISTANI EMBASSY IN KABUL, 2003-07-08 (photo)

Ahmad Masood

REU7791448

AFGHAN PROTESTERS SHOUT ANTI-PAKISTAN SLOGANS IN KABUL., 2003-07-08 (photo)
 
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AFGHAN PROTESTERS SHOUT ANTI-PAKISTAN SLOGANS IN KABUL., 2003-07-08 (photo)

Ahmad Masood

REU7589508

AFGHAN PROTESTERS SHOUT ANTI-PAKISTAN SLOGANS IN KABUL., 2003-07-08 (photo)

Ahmad Masood

REU7589508

CROTONE COUNTRYSIDE - PIGS GRAZING IN FRONT OF THE HOUSE, 1954 (photo)
 
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CROTONE COUNTRYSIDE - PIGS GRAZING IN FRONT OF THE HOUSE, 1954 (photo)

Gilardi, Ando (1921-2012)

FGL11857533

CROTONE COUNTRYSIDE - PIGS GRAZING IN FRONT OF THE HOUSE, 1954 (photo)

Gilardi, Ando (1921-2012)

FGL11857533

CROTONE COUNTRYSIDE - A ROOF OVER YOUR HEAD, 1954 (photo)
 
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CROTONE COUNTRYSIDE - A ROOF OVER YOUR HEAD, 1954 (photo)

Gilardi, Ando (1921-2012)

FGL11857557

CROTONE COUNTRYSIDE - A ROOF OVER YOUR HEAD, 1954 (photo)

Gilardi, Ando (1921-2012)

FGL11857557

CROTONE COUNTRYSIDE - IANNELLI VILLAGE, , 1954 (photo)
 
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CROTONE COUNTRYSIDE - IANNELLI VILLAGE, , 1954 (photo)

Gilardi, Ando (1921-2012)

FGL11856853

CROTONE COUNTRYSIDE - IANNELLI VILLAGE, , 1954 (photo)

Gilardi, Ando (1921-2012)

FGL11856853

CROTONE COUNTRYSIDE - A ROOF OVER YOUR HEAD, , 1954 (photo)
 
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CROTONE COUNTRYSIDE - A ROOF OVER YOUR HEAD, , 1954 (photo)

Gilardi, Ando (1921-2012)

FGL11856842

CROTONE COUNTRYSIDE - A ROOF OVER YOUR HEAD, , 1954 (photo)

Gilardi, Ando (1921-2012)

FGL11856842

CROTONE COUNTRYSIDE - HOUSE UNDER CONSTRUCTION, , 1954 (photo)
 
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CROTONE COUNTRYSIDE - HOUSE UNDER CONSTRUCTION, , 1954 (photo)

Gilardi, Ando (1921-2012)

FGL11856857

CROTONE COUNTRYSIDE - HOUSE UNDER CONSTRUCTION, , 1954 (photo)

Gilardi, Ando (1921-2012)

FGL11856857

CROTONE COUNTRYSIDE - FINALLY THE ROOF!, 1954 (photo)
 
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CROTONE COUNTRYSIDE - FINALLY THE ROOF!, 1954 (photo)

Gilardi, Ando (1921-2012)

FGL11857566

CROTONE COUNTRYSIDE - FINALLY THE ROOF!, 1954 (photo)

Gilardi, Ando (1921-2012)

FGL11857566

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