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Immagini di 'Radio Scoperto' trovate, 21

Pierre Curie (1859-1906) teaching about radium at the Sorbonne, 1906 (b/w photo)

Pierre Curie (1859-1906) teaching about radium at the Sorbonne, 1906 (b/w photo)

French Photographer, (20th century)

CHT237253

Pierre Curie (1859-1906) (b/w photo)

Pierre Curie (1859-1906) (b/w photo)

French Photographer, (20th century)

ACD237252

William Ramsay explains to Pierre Curie, who discovered radium, his studies on the transformation of radium into helium.

William Ramsay explains to Pierre Curie, who discovered radium, his studies on the transformation of radium into helium.

Unknown Artist, (20th century)

Giancarlo Costa

GIA4733731

Pierre (1859-1906) and Marie Curie (1867-1934) in their laboratory, c.1903 (b/w photo)

Pierre (1859-1906) and Marie Curie (1867-1934) in their laboratory, c.1903 (b/w photo)

French Photographer, (20th century)

CHT237251

Caricature of Pierre and Marie Sklodowska Curie, who discovered radium and polonium. c. 1900

Caricature of Pierre and Marie Sklodowska Curie, who discovered radium and polonium. c. 1900

EVB2936693

Two views of the shed at the School of Physics on the Rue Lhomond where radium was discovered (b/w photo)

Two views of the shed at the School of Physics on the Rue Lhomond where radium was discovered (b/w photo)

European Photographer, (20th century)

LLM3650370

Portrait of Marie Curie (1867-1934) and her Daughter, Irene Joliot-Curie (1897-1956) in their Laboratory in 1924, from 'Le Monde Illustre' (b/w photo)

Portrait of Marie Curie (1867-1934) and her Daughter, Irene Joliot-Curie (1897-1956) in their Laboratory in 1924, from 'Le Monde Illustre' (b/w photo)

French School, (20th century)

CHT173241

Paris, France: December 26, 1923
A portrait of Marie Curie, who with her husband, discovered radium. — Paris, France: December 26, 1923 A portrait of Marie Curie, who with her husband, discovered radium.

Paris, France: December 26, 1923 A portrait of Marie Curie, who with her husband, discovered radium.

UIG5447628

Marie Curie (1867-1934) Giving a Lecture in her Laboratory (b/w photo)

Marie Curie (1867-1934) Giving a Lecture in her Laboratory (b/w photo)

French School, (20th century)

CHT173244

Portrait of Marie Curie (1867-1934) (b/w photo)

Portrait of Marie Curie (1867-1934) (b/w photo)

French School, (20th century)

ACD173245

Radio Equipment, Transmitters SWB1 short-wave radio transmitter no 7, 1927

Radio Equipment, Transmitters SWB1 short-wave radio transmitter no 7, 1927

UIS5082365

Gugliemo Marconi, Italian radio pioneer, c 1920

Gugliemo Marconi, Italian radio pioneer, c 1920

UIS5075726

Radio Communications, 1886-1939 Apparatus used by Heinrich Hertz, c 1887

Radio Communications, 1886-1939 Apparatus used by Heinrich Hertz, c 1887

UIS5069700

Pierre Curie chatting with Sir William Ramsay (litho)

Pierre Curie chatting with Sir William Ramsay (litho)

STC335871

RADIO COMMUNICATIONS, 1886-1939 Hertz rectangular oscillator, c 1888

RADIO COMMUNICATIONS, 1886-1939 Hertz rectangular oscillator, c 1888

UIS5064536

SECURITY OFFICIALS DISPLAY RADIO SIGNAL HANDSETS IN SRINAGAR, 2002-05-20 (photo)

SECURITY OFFICIALS DISPLAY RADIO SIGNAL HANDSETS IN SRINAGAR, 2002-05-20 (photo)

Altaf Hussain

REU8020282

Wife slapping her cheating husband, Italy, 1966 (b/w photo)

Wife slapping her cheating husband, Italy, 1966 (b/w photo)

Sergio del Grande

MEP3110628

Our galaxy -Artist's view - Our galaxy, the Milky Way - Artwork - Representation of our galaxy, the lactee path, with the position of our Sun. Following observations made in infrared by the Spitzer space telescope, astronomers believe that our galaxy is a spiral galaxy consisting of two main arms (Scutum-Centaurus and Perseus) visible from the extremities of a large central bar. Two smaller arms (Norma and Sagittarius) are located between the main arms. The main arms contain the highest densities in stars, the other two are essentially gas. A new spiral arm, called the arm of the kiloparsec Far-3, runs along the bar of the galaxy. Our sun is close to a small interrupted arm called Orion's arm, located between the arms of Sagittarius and Persee. The Lactee Way was previously thought to have four main arms. Using infrared images from Nasa's Spitzer Space Telescope, scientists have discovered that the Milky Way's elegant spiral structure is dominated by just two arms wrapping off the ends of a central bar of stars. Previously, our galaxy was thought to possess four major arms. This artist's concept illustrates the new view of the Milky Way, along with other findings presented at the 212th American Astronomical Society meeting in St. Louis, Mo. The galaxy's two major arms (Scutum-Centaurus and Perseus) can be seen attached to the ends of a thick central bar, while the two now-demoted minor arms (Norma and Sagittarius) are less distinct and located between the major arms. The major arms consist of the highest densities of both young and old stars; the minor arms are primarily filled with gas and pockets of star-forming activity. The artist's concept also includes a new spiral arm, called the “Far-3 kiloparsec arm,””” discovered via a radio-telescope survey of gas in the Milky Way. This arm is shorter than the two major arms and li — Our galaxy -Artist's view - Our galaxy, the Milky Way - Artwork - Representation of our galaxy, the lactee path, with the position of our Sun. Following observations made in infrared by the Spitzer space telescope, astronomers believe that our galaxy is a spiral galaxy consisting of two main arms (Scutum-Centaurus and Perseus) visible from the extremities of a large central bar. Two smaller arms (Norma and Sagittarius) are located between the main arms. The main arms contain the highest densities in stars, the other two are essentially gas. A new spiral arm, called the arm of the kiloparsec Far-3, runs along the bar of the galaxy. Our sun is close to a small interrupted arm called Orion's arm, located between the arms of Sagittarius and Persee. The Lactee Way was previously thought to have four main arms. Using infrared images from Nasa's Spitzer Space Telescope, scientists have discovered that the Milky Way's elegant spiral structure is dominated by just two arms wrapping off the ends

Our galaxy -Artist's view - Our galaxy, the Milky Way - Artwork - Representation of our galaxy, the lactee path, with the position of our Sun. Following observations made in infrared by the Spitzer space telescope, astronomers believe that our galaxy is a spiral galaxy consisting of two main arms (Scutum-Centaurus and Perseus) visible from the extremities of a large central bar. Two smaller arms (Norma and Sagittarius) are located between the main arms. The main arms contain the highest densities in stars, the other two are essentially gas. A new spiral arm, called the arm of the kiloparsec Far-3, runs along the bar of the galaxy. Our sun is close to a small interrupted arm called Orion's arm, located between the arms of Sagittarius and Persee. The Lactee Way was previously thought to have four main arms. Using infrared images from Nasa's Spitzer Space Telescope, scientists have discovered that the Milky Way's elegant spiral structure is dominated by just two arms wrapping off the ends

PIX4638218

Persee Galaxy Cluster - Perseus galaxy cluster - The Persee galaxy cluster (Abell 426) contains at least 500 galaxies including the large elliptical galaxy NGC 1275. This galaxy (the galaxy with pink filaments to the left of the image) is located about 235 million years ago - light; it is a very strong source of radio wave transmission known as Perseus A. In the right center of the image, note the presence of a supernova, SN 2008fg, in a small blue spiral galaxy, NGC 1268. Perseus galaxy cluster (Abell 426) is a cluster of about 500 galaxies. The biggest (left) is NGC 1275, located 235 million light years away; it is a strong radio source known as Perseus A. The gravity exerted by the luminous parts of a galaxy cluster is insufficient to hold the cluster together. Thus, scientists have concluded the missing adhesive must be dark matter and since it's invisible to modern instruments - it can only be inferred. So, when one views the image of the Perseus Galaxy Cluster, ones sees only a small fraction of what's actually there. This image was serendipitously exposed during the brief appearance of a supernova, designated SN2008FG, in one of the small blue spiral galaxies caught in the field of view (center right). It was discovered on August 30, 2008 by the 30 - inch KAIT robotic supernova patrol telescope located at historic Lick Observatory near San Jose, California. The stellar explosion, characterized by its bright blue color, is located near the bottom right edge of the galaxy. This cataclysmic event easily outshines the combined light of its home star system, NGC 1268 — Persee Galaxy Cluster - Perseus galaxy cluster - The Persee galaxy cluster (Abell 426) contains at least 500 galaxies including the large elliptical galaxy NGC 1275. This galaxy (the galaxy with pink filaments to the left of the image) is located about 235 million years ago - light; it is a very strong source of radio wave transmission known as Perseus A. In the right center of the image, note the presence of a supernova, SN 2008fg, in a small blue spiral galaxy, NGC 1268. Perseus galaxy cluster (Abell 426) is a cluster of about 500 galaxies. The biggest (left) is NGC 1275, located 235 million light years away; it is a strong radio source known as Perseus A. The gravity exerted by the luminous parts of a galaxy cluster is insufficient to hold the cluster together. Thus, scientists have concluded the missing adhesive must be dark matter and since it's invisible to modern instruments - it can only be inferred. So, when one views the image of the Perseus Galaxy Cluster, ones sees only a s

Persee Galaxy Cluster - Perseus galaxy cluster - The Persee galaxy cluster (Abell 426) contains at least 500 galaxies including the large elliptical galaxy NGC 1275. This galaxy (the galaxy with pink filaments to the left of the image) is located about 235 million years ago - light; it is a very strong source of radio wave transmission known as Perseus A. In the right center of the image, note the presence of a supernova, SN 2008fg, in a small blue spiral galaxy, NGC 1268. Perseus galaxy cluster (Abell 426) is a cluster of about 500 galaxies. The biggest (left) is NGC 1275, located 235 million light years away; it is a strong radio source known as Perseus A. The gravity exerted by the luminous parts of a galaxy cluster is insufficient to hold the cluster together. Thus, scientists have concluded the missing adhesive must be dark matter and since it's invisible to modern instruments - it can only be inferred. So, when one views the image of the Perseus Galaxy Cluster, ones sees only a s

R. Jay GaBany

PIX4565332

Our galaxy-position of the Sun -Artist's view - Our galaxy, the Milky Way - Artwork - Representation of our galaxy, the lactee path, with the position of our Sun. Following observations made in infrared by the Spitzer space telescope, astronomers believe that our galaxy is a spiral galaxy consisting of two main arms (Scutum-Centaurus and Perseus) visible from the extremities of a large central bar. Two smaller arms (Norma and Sagittarius) are located between the main arms. The main arms contain the highest densities in stars, the other two are essentially gas. A new spiral arm, called the arm of the kiloparsec Far-3, runs along the bar of the galaxy. Our sun is close to a small interrupted arm called Orion's arm, located between the arms of Sagittarius and Persee. The Lactee Way was previously thought to have four main arms. Using infrared images from Nasa's Spitzer Space Telescope, scientists have discovered that the Milky Way's elegant spiral structure is dominated by just two arms wrapping off the ends of a central bar of stars. Previously, our galaxy was thought to possess four major arms. This annotated artist's concept illustrates the new view of the Milky Way, along with other findings presented at the 212th American Astronomical Society meeting in St. Louis, Mo. The galaxy's two major arms (Scutum-Centaurus and Perseus) can be seen attached to the ends of a thick central bar, while the two now-demoted minor arms (Norma and Sagittarius) are less distinct and located between the major arms. The major arms consist of the highest densities of both young and old stars; the minor arms are primarily filled with gas and pockets of star-forming activity. The artist's concept also includes a new spiral arm, called the “Far-3 kiloparsec arm,””” discovered via a radio-telescope survey of gas in the Milky Way. This arm is shorter t — Our galaxy-position of the Sun -Artist's view - Our galaxy, the Milky Way - Artwork - Representation of our galaxy, the lactee path, with the position of our Sun. Following observations made in infrared by the Spitzer space telescope, astronomers believe that our galaxy is a spiral galaxy consisting of two main arms (Scutum-Centaurus and Perseus) visible from the extremities of a large central bar. Two smaller arms (Norma and Sagittarius) are located between the main arms. The main arms contain the highest densities in stars, the other two are essentially gas. A new spiral arm, called the arm of the kiloparsec Far-3, runs along the bar of the galaxy. Our sun is close to a small interrupted arm called Orion's arm, located between the arms of Sagittarius and Persee. The Lactee Way was previously thought to have four main arms. Using infrared images from Nasa's Spitzer Space Telescope, scientists have discovered that the Milky Way's elegant spiral structure is dominated by just two arms w

Our galaxy-position of the Sun -Artist's view - Our galaxy, the Milky Way - Artwork - Representation of our galaxy, the lactee path, with the position of our Sun. Following observations made in infrared by the Spitzer space telescope, astronomers believe that our galaxy is a spiral galaxy consisting of two main arms (Scutum-Centaurus and Perseus) visible from the extremities of a large central bar. Two smaller arms (Norma and Sagittarius) are located between the main arms. The main arms contain the highest densities in stars, the other two are essentially gas. A new spiral arm, called the arm of the kiloparsec Far-3, runs along the bar of the galaxy. Our sun is close to a small interrupted arm called Orion's arm, located between the arms of Sagittarius and Persee. The Lactee Way was previously thought to have four main arms. Using infrared images from Nasa's Spitzer Space Telescope, scientists have discovered that the Milky Way's elegant spiral structure is dominated by just two arms w

PIX4638214

Alt! Mines in sight! (colour litho)

Alt! Mines in sight! (colour litho)

Beltrame, Achille (1871-1945)

LLM2783950

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