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Georges Auric And Jacqueline Rayet At The Repetition Of “Turan-Galila” At L'Opera In 1968 (b/w photo)
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Artist's view of a Wolf Star - Rayet - Artwork of a Wolf - Rayet star - Wolf Stars - Rayet are extremely massive stars that lose their material under the influence of a powerful stellar wind. A Wolf - Rayet star in its final hours. Wolf - Rayet stars are extremely massive bluish stars, containing the mass of 10 to 15 suns. The blue - white color of the star indicates that its surface temperature is approximately 50,000 C. Surrounding the star are wisps of gas that have recently been shed from the outer atmosphere
cars years 30 Sizaire and Naudin and Rayet-Lienart
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Portrait of the first dancer Jacqueline Rayet (born 1933) in 1956
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Portrait of the first dancer Jacqueline Rayet (born 1933) in 1956
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Nebula NGC 7635 in Cassiopee - The Bubble Nebula (NGC 7635) in Cassiopeia - This nebula is located about 7100 years - light from Earth. A star 40 times more massive than our Sun, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. The Bubble Nebula in Cassiopeia is one of the most dramatic emission nebulae visible in the northern hemisphere. Lying at a distance of about 7,000 light - years away and spanning six light - years in diameter, NGC 7635 is quite bright with a magnitude of 7.0. The star in the middle of the bubble, BD+602522, is responsible for this stunning site, for this very hot star emits so much UV radiation that it is able to also heat and excite the surrounding dust and gas, thus emitting its own radiation. It is a Wolf - Rayet star, a very luminous star and also very short - lived. This Wolf - Rayet star is 40 times as massive than our sun
Nebula of the crescent NGC 6888 in the Swan - Crescent nebula in Cygnus - NGC 6888, the nebula of the Crescent. This nebula is a gas shell located in the constellation Swan. The bright star in the center of the nebula is the star WR 136, a star of Wolf - Rayet, massive, very hot. The nebula NGC 6888 is a shell of gas that is being energized by the strong stellar wind from the Wolf - Rayet star WR 136, the bright star at the center of the nebula. It is located in the constellation of Cygnus, the Swan. Wolf - Rayet stars are very hot, massive stars that are blowing off their outer layers
Nebula of the crescent NGC 6888 in the Swan - NGC 6888 The Crescent Nebula - NGC 6888 Nebula of the Crescent. This nebula is a gas shell located in the constellation Swan. The bright star in the center of the nebula is the star WR 136, a star of Wolf - Rayet, massive, very hot. The nebula is a shell of gas that is being energized by the strong stellar wind from the Wolf - Rayet star WR 136, the bright star at the center of the nebula. It is located in the constellation of Cygnus, the Swan. Wolf - Rayet stars are very hot, massive stars that are blowing off their outer layers
Nebula NGC 2359 in the Big Dog - NGC 2359 nebula in Canis Major - NGC 2359 is a nebula in the Big Dog that houses a star Wolf - Rayet, HD 56925. NGC 2359 (Thor's Helmet) is a prototypical wind blown bubble powered by the extremely massive and unstable Wolf - Rayet star HD 56925. These types of stars (only about 300 are known presently) represent a late evolutionary phase of massive O - type blue giants which have become unstable in the late stages of their short stellar life
Nebula NGC 7635 in Cassiopee - Bubble Nebula (NGC 7635) in Cassiopeia - This nebula is located about 7100 years - light from Earth. A massive star, called Wolf - Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. The Bubble Nebula in Cassiopeia is one of the most dramatic emission nebulae visible in the northern hemisphere. Lying at a distance of about 7,000 light - years away and spanning six light - years in diameter, NGC 7635 is quite bright with a magnitude of 7.0. The star in the middle of the bubble, BD+602522, is responsible for this stunning site, for this very hot star emits so much UV radiation that it is able to also heat and excite the surrounding dust and gas, thus emitting its own radiation. It is a Wolf - Rayet star, a very luminous star and also very short - lived. This Wolf - Rayet star is 40 times as massive than our sun
Stellar black hole - Artist's view - A stellar black hole - Artist's view of a system composed of a Wolf-Rayet star orbiting a black hole. A stellar black hole is born from the gravitational collapse of a massive star. The stellar black holes have a mass of some solar masses. A black hole is a region of space whose gravitation is so strong that it will prevent any form of material or radiation from escaping. This artist's impression depicts a star-mass black hole. The black hole has a mass of about twenty times the mass of the Sun and is associated with a Wolf-Rayet star: a star that will become a black hole itself. The black hole is stripping matter away from the star as they orbit each other
Open cluster Westerlund 2 in Carene - Open cluster Westerlund 2 in Carina - The open cluster Westerlund 2 is located about 20,000 years - light in the southern constellation of Carene, within the nebula Gum 29. About 3000 stars form this cluster. It contains a significant number of massive stars including one of the most massive stars known to date: WR 20a. Image obtained by the Hubble Space Telescope. The sparkling centerpiece of this image taken by the Hubble space telescope is a giant cluster of about 3,000 stars called Westerlund 2, named for Swedish astronomer Bengt Westerlund, who discovered the grouping in the 1960s. The cluster resides in a raucous stellar breeding ground known as Gum 29, located 20,000 light - years away from Earth in the constellation Carina. To capture this image, Hubble's near - infrared Wide Field Camera 3 near - infrared pierced through the dusty veil shrouding the stellar nursery, giving astronomers a clear view of the nebula and the dense concentration of stars in the central cluster. The cluster measures between 6 to 13 light - years across. The giant star cluster is only about 2 million years old and contains some of our galaxy's hottest, brightest, and most massive stars. Some of its heftiest stars unleash torrents of ultraviolet light and hurricane - force winds of charged particles that etch at the enveloping hydrogen gas cloud. The nebula reveals a fantasy landscape of pillars, ridges, and valleys. The pillars, composed of dense gas and thought to be incubators for new stars are a few light - years tall and point to the central star cluster. Other dense regions surround the pillars, including reddish - brown filaments of gas and dust. The brilliant stars sculpt the gaseous terrain of the nebula and help create a successive generation of baby stars. When the stellar winds hit dense walls of gas, the shockwaves may spark a new torrent of star birth along the wall of the cavity. The red dots scattered t
Nebula in the galaxy NGC 6822 - Bubble nebulae in NGC 6822 - Nebula in the irregular galaxy NGC 6822, adjacent to our galaxy. This gas bubble houses massive stars known as Wolf - Rayet. NGC 6822 is a nearby irregular galaxy reminiscent of the Large Magellanic Cloud (LMC). Like the LMC it contains many, extremely hot stars of the Wolf - Rayet type, stars which often have intense stellar winds blasting from their surfaces. Small groups of such stars are found at the centres of the bubble nebulae seen here, which are the result of the stellar winds colliding with the more or less stationary interstellar medium in NGC 6822. At the interface of the collision, the interstellar medium glows, producing a thin, luminous bubble. Such bubbles are rare in the more turbulent Milky Way galaxy, but Henize 70 in the Large Magellanic Cloud is similar
Nebula of the crescent NGC 6888 in the Swan - Crescent nebula in Cygnus - NGC 6888 the nebula of the Crescent. This nebula is a gas shell located in the constellation Swan. The bright star in the center of the nebula is the star WR 136, a star of Wolf - Rayet, massive, very hot. The nebula is a shell of gas that is being energized by the strong stellar wind from the Wolf - Rayet star WR 136, the bright star at the center of the nebula. It is located about 5,000 light years from Earth in the constellation of Cygnus, the Swan. Wolf - Rayet stars are very hot, massive stars that are blowing off their outer layers
Nebula NGC 7635 in Cassiopee - The Bubble Nebula: This nebula is located about 8000 light years from Earth. A star 40 times more massive than our Sun, called Wolf-Rayet, is responsible for the formation of this bubble; it is the star BD+60* 2522. Image obtained by the space telescope Hubble - The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away - This complete view of the Bubble Nebula allows us to fully appreciate the almost perfectly symmetrical shell which gives the nebula its name. This shell is the result of a powerful flow of gas - known as a stellar wind - from the bright star visible just to the left of centre in this image. The star, SAO 20575, is between ten and twenty times the mass of the Sun and the pressure created by its stellar wind forces the surrounding interstellar material outwards into this bubble-like form - The giant molecular cloud that surrounds the star - glowing in the star's intense ultraviolet radiation - tries to stop the expansion of the bubble. However, although the sphere already measures around ten light-years in diameter, it is still growing, owing to the constant pressure of the stellar wind - currently at more than 100,000 kilometers per hour! - This stunning new image was observed by the NASA/ESA Hubble Space Telescope
Nebula NGC 2359 in the Grand Chie
Nebula of the crescent NGC 6888 in the Swan - NGC 6888 Crescent Nebula - NGC 6888 Nebula of the Crescent. This nebula is a gas shell located in the constellation Swan. The bright star in the center of the nebula is the star WR 136, a star of Wolf - Rayet, massive, very hot. Image obtained by combining light through 3 different filters that highlight oxygen, hydrogen, and sulfur. The nebula is a shell of gas that is being energized by the strong stellar wind from the Wolf - Rayet star WR 136, the bright star at the center of the nebula. It is located in the constellation of Cygnus, the Swan. Wolf - Rayet stars are very hot, massive stars that are blowing off their outer layers. Narrowband false color composite H - alpha, OIII, SII
ngc2359 - NGC2359 Star Wolf Raye
Nebula NGC 2359 in the Big Dog - NGC 2359 is a nebula in the Big Dog that houses a star Wolf - Rayet, HD 56925
Nebula NGC 2359 in the Great Dog - NGC 2359 nebula in Canis Major - NGC 2359 is a nebula located about 15 000 years - light from Earth, in the constellation Big Dog. It houses a star Wolf - Rayet, HD 56925. NGC 2359 (Thor's Helmet) is a prototypical wind blown bubble powered by the extremely massive and unstable Wolf - Rayet star HD 56925. These types of stars (only about 300 are known presently) represent a late evolutionary phase of massive O - type blue giants which have become unstable in the late stages of their short stellar life
Nebula NGC 2359 in the Big Dog - A Wolf - Rayet star in NGC 2359 - NGC 2359 is a nebula in the Big Dog that houses a star Wolf - Rayet, HD 56925. Image obtained by Siding Spring's 3.9m telescope. NGC 2359 is the nebula produced by a single, extremely hot star HD 56925. This is one of the rare Wolf - Rayet stars, whose intrinsic brilliance is combined with high rates of mass loss from its surface. This material is ejected from the star with velocities which approach 2000 kilometers per second. This violent activity quickly reduces the mass of the star which in turn reduces the instability. The rapidly - moving ejected material interacts with the gas and dust around the star producing the cosmic bubble seen here. Such stars are unusual, largely because extreme behaviour of this kind cannot be sustained for long. This particular example is spectacular because it happens to inhabit a part of our Galaxy rich in interstellar gas
Nebula IC 1318 in the Swan - Gamma Cygnus, IC 1318, NGC 6888 - IC 1318 is a very extended emission nebula that surrounds the star Gamma Cygni (Sadr), visible towards the middle of the image. Lower right is the nebula NGC 6888 which surrounds a star Wolf - Rayet. This complex of red emission nebulosity in Cygnus surrounds the bright 2.2 magnitude star Gamma Cygni, or Sadr, just above right of the center of the frame. Above Sadr are two patches of nebulosity designated as IC 1318, popularly called the Butterfly Nebula. At the lower left of the frame is NGC 6888, the Crescent Nebula, a very interesting nebula that surrounds a Wolf - Rayet star
Nebula NGC 3603 in Carene - Star formation region NGC 3603 in Carina - NGC 3603 is located about 7000 years - light from Earth in the constellation Carene. Within this nebula, a cluster of massive stars, Wolf - Rayet stars. Image obtained by Siding Spring's 3.9m telescope. Although stars are well known to form in clusters, most of the stars in the young groups we know of in our own galaxy are well separated in space. In NGC 3603 the stars are remarkably close together. Moreover, many of the stars in this compact constellation are Wolf - Rayet stars, extremely hot, massive objects, rarely found in such profusion in clusters. Exactly why some clusters form massive stars and others do not is a hot topic in astronomy, so this cluster and its environment has been extensively studied. This curious collection of young objects is, as far as we know, unique in our galaxy, though the enigmatic object at the centre of the Tarantula Nebula in the Large Magellanic Cloud is now known to be a similar compact cluster. The stars and their associated nebula are seen through considerable dust along the line of sight, and are dimmed and reddened by it
Massive stars in the Carene - Massive stars in the Carina Nebula - Detail of the nebula of the Carene, located about 7500 years ago - light from Earth, obtained by the Hubble space telescope. The image shows down the image a cluster of stars named Trumpler 16 which contains two very massive stars, WR 25 at Tr16 - 244. The image shows a pair of colossal stars, WR 25 and Tr16 - 244, located within the open cluster Trumpler 16, at the bottom of the image. This cluster is embedded within the Carina Nebula, an immense cauldron of gas and dust that lies approximately 7500 light - years from Earth in the constellation of Carina, the Keel. At the top of the image, a peculiar nebula with the shape of a “” defiant”” finger points towards WR25 and Tr16 - 244
Dancers Jacqueline Rayet and Jean Pierre Bonnefous during Rehearsal of "Webern Opus 5" at The "Opera De Paris", April 29, 1967 (b/w photo)
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Massive Stars in the Carene - Massive stars in the Carina Nebula - The image shows a cluster of stars named Trumpler 16 which contains two very massive stars, WR 25 at Tr16 - 244. WR 25 is the brightest star on the image. It is a double star composed of a star at least 50 times more massive than the Sun. Tr16 - 244 is the third brightest star in this image (top left of WR 25). It's a triple star. The second bright star in the image, to the left of WR 25, is a small star, which does not belong to this cluster and is located much closer to us. The Carene Nebula is located about 7500 years from Earth
Nebula IC 1318 in the Swan - Gamma Cygnus, IC 1318, NGC 6888 - IC 1318 is a very extended emission nebula that surrounds the star Gamma Cygni (Sadr), visible towards the middle of the image. Lower right is the nebula NGC 6888 which surrounds a star Wolf - Rayet. This large area of emission nebulosity surrounds Sadr, Gamma Cygni, the brightest star in this photo and the heart of the constellation of Cygnus the Swan. Numerous star clusters can also be found embedded in the nebulosity. The two sections of nebulosity to the left of Sadr are called the Butterfly Nebula, and have the catalog designation of IC 1318. The large area of dark nebulosity that separates the two halves of the Butterfly is LDN 889, and B343 is the small but very dense dark nebula at the center right of the image. The small open cluster NGC 6910 is just above Sadr. The Crescent Nebula, NGC 6888, is at the lower right. The small patches of blue reflection nebulosity at top left are part of the NGC 6914/van den Berg 131/van den Berg 132 complex
Star cluster in the nebula NGC 3603 - Star cluster in NGC 3603 nebula - Cluster of young stars in the nebula NGC 3603, located about 20,000 years ago - light from Earth in the southern constellation of Carene. Image obtained by the Hubble Space Telescope in August and December 2009. NGC 3603 is a prominent star - forming region located in the Carina spiral arm of the Milky Way, about 20,000 light - years away from our Solar System. This image from the NASA/ESA Hubble Space Telescope shows a young star cluster surrounded by a vast region of dust and gas. Most of the bright stars in the image are hot blue stars whose ultraviolet radiation and violent winds have blown out an enormous cavity in the gas and dust enveloping the cluster. This Hubble Space Telescope image was captured in August 2009 and December 2009 with the Wide Field Camera 3 in both visible and infrared light, which trace the glow of sulfur, hydrogen, and iron
Nebula NGC 3372 in the Carene - Carina nebula NGC 3372 - The Carene nebula is located about 7500 years from the Earth. It is home to many hot stars, including the massive star Eta Carinae at the bottom left of the image, the clusters of young stars Trumpler 14 (above the right of eta carinae) and Collinder 228 (below eta carinae). To the right of the image, the bright star is WR 22, a star Wolf - Rayet. Image obtained by the 2.2m ESO/MPG telescope of the La Silla Observatory in Chile. This spectacular panoramic view combines a new image of the field around the Wolf - Rayet star WR 22 in the Carina Nebula (right) with an earlier picture of the region around the unique star Eta Carinae in the heart of the nebula (left). The picture was created from images taken with the Wide Field Imager on the MPG/ESO 2.2 - metre telescope at Eso's La Silla Observatory in Chile
Nebula N70 in the Great Magellan Cloud - The N 70 nebula in Large Magellanic Cloud (LMC) - The Henize 70 nebula extends for about 400 years - light, it is located in the Great Magellan Cloud. In the center, a small group of very massive and extremely hot stars, stars of Wolf - Rayet. Image obtained by Siding Spring's 3.9m telescope. At the centre of this remarkable bubble - like nebula nebula is a small group of extremely hot stars. Some of these stars are rapdly losing mass and have stellar winds blowing from their surfaces with velocities that approach 4000 kilometers per second. Such stars are known as Wolf - Rayet stars and are found in galaxies capable of forming massive stars. There are many such stars in the Large Magellanic Cloud (LMC) but not all of them are associated with distinctive nebulae. The outward flowing streams of energetic particles from Wolf - Rayet (and other energetic stars) eventually interact with the relatively stationary interstellar medium pervading the LMC, releasing much of their energy as a thin spherical shell of luminous material. The hollow structure accounts for the shape we see in the sky. This nebula is almost 400 light years across, about 100 times the distance from the Sun to the nearest star. The LMC is about 160,000 light years away and is the closest galaxy to the Milky Way
Dancers Jacqueline Rayet and Lucien Duthoit in Ballet "Petrouchka" at Paris Opera on December 17, 1964 (b/w photo)
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Nebula N70 in the Great Magellan Cloud - The N 70 nebula in Large Magellanic Cloud (LMC) - The Henize 70 nebula extends for about 400 years - light, it is located in the Great Magellan Cloud. In the center, a small group of very massive and extremely hot stars, stars of Wolf - Rayet. Image obtained by Siding Spring's 3.9m telescope. At the centre of this remarkable bubble - like nebula nebula is a small group of extremely hot stars. Some of these stars are rapdly losing mass and have stellar winds blowing from their surfaces with velocities that approach 4000 kilometers per second. Such stars are known as Wolf - Rayet stars and are found in galaxies capable of forming massive stars. There are many such stars in the Large Magellanic Cloud (LMC) but not all of them are associated with distinctive nebulae. The outward flowing streams of energetic particles from Wolf - Rayet (and other energetic stars) eventually interact with the relatively stationary interstellar medium pervading the LMC, releasing much of their energy as a thin spherical shell of luminous material. The hollow structure accounts for the shape we see in the sky. This nebula is almost 400 light years across, about 100 times the distance from the Sun to the nearest star. The LMC is about 160,000 light years away and is the closest galaxy to the Milky Way
Detail of the nebula NGC 3603 in the Carene - Star life cycle in NGC 3603 - In the center of the picture is a cluster of massive young stars formed from the gas surrounding them. Two pillars of gas and dust visible on the right at the top and bottom will one day form other stars, as probably the dark cloud at the top right of the image called Bok's globule. Above the left of the star cluster, an old blue supergiant star, Sher 25, arrives at the end of life. The nebula NGC 3603 is located approximately 20,000 light years from Earth in the southern constellation of Carene. Image obtained by the Hubble Space Telescope. This image made by the Hubble space telescope nicely illustrates the entire stellar life cycle of stars, starting with the Bok globules (dark clouds at the upper right) and giant gaseous pillars, followed by circumstellar disks and progressing to evolved massive stars in the young starburst cluster (center). The blue supergiant star Sher 25 with its ring and bipolar outflow (upper left of center) marks the end of the life cycle. NGC 3603 is located 20 000 light years away in Carina constellation
French Dancer Jacqueline Rayet in Ballet "Petrouchka" in Ballet "Petrouchka" Paris Opera on December 17, 1964 (b/w photo)
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French dancer Jacqueline Rayet, new prima ballerina at the Paris Opera, December 25, 1960 (b/w photo)
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Star cluster in the nebula NGC 3603 - Star cluster in NGC 3603 nebula - Cluster of young stars in the nebula NGC 3603, located about 20,000 years ago - light from Earth in the southern constellation of Carene. Image obtained by the Hubble Space Telescope on 29 December 2005. NGC 3603 is a prominent star - forming region located in the Carina spiral arm of the Milky Way, about 20,000 light - years away from our Solar System. This image from the NASA/ESA Hubble Space Telescope shows a young star cluster surrounded by a vast region of dust and gas. Most of the bright stars in the image are hot blue stars whose ultraviolet radiation and violent winds have blown out an enormous cavity in the gas and dust enveloping the cluster
Maurice Bejart during Rehearsal of Ballet "Le Sacre Du Printemps" April 22, 1965, in The C : Jacqueline Rayet and Cyril Athanassof (photo)
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Dario Moreno With Emmanuelle Riva and Jacqueline Rayet at Premiere of Film Marnie in Paris November 7, 1964 (b/w photo)
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Rehearsal of Ballet "Le Sacre Du Printemps" By Maurice Bejart, in The C Is Jacqueline Rayet, April 22, 1965 (b/w photo)
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Gamma Velorum - Gamma Velorum - Gamma Velorum is the brightest star in the southern constellation Sails. It's a Wolf - Rayet star associated with a blue star. Wolf - Rayet stars are extremely massive stars that lose their material by a powerful stellar wind. At the bottom of the picture, the open cluster NGC 2547. Gamma Velorum in the constellation Vela is the brightest Wolf - Rayet star in the sky. These stars have masses 10 - 50 times larger than our sun. Also visible at bottom right is open cluster NGC 2547
Maurice Bejart and Jacqueline Rayet during Rehearsals of Ballet "Le Sacre Du Printemps" at Paris Opera April 22, 1965 (b/w photo)
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George Balanchine (1904-1983) Russian Choreographer and Ballet Master during Rehearsal With Jacqueline Rayet at Paris Opera House December 17, 1963  (b/w photo)
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Dancers Jacqueline Rayet and Cyril Athanassof during Rehearsal of Ballet "Le Sacre Du Printemps" at Opera De Paris, April 21, 1965 (b/w photo)
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At The International Dance Festival in Paris : Claude Pompidou (R) With A Dancer of Paris Opera Jacqueline Rayet Under Look of Michel Guy on November 3, 1967 (b/w photo)
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Cliff Edwards (1895-1971) American singer and voice actor, also known as 'Ukulele Ike ' Aboard a yacht in the Hudson River with Frank Raye 1947 (b/w photo)
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George Balanchine (1904-1983) Russian Choreographer and Ballet Master during Rehearsal For Ballet "Bourree Fantasque" With Dancer Jacqueline Rayet at Paris Opera House December 17, 1963 (b/w photo)
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French Choreographer Roland Petit With his Dancers : L-R : Jacqueline Rayet, Christiane Vlassi, Georges Piletta, Nanon Thibon and Claire Motte June 19, 1968 (b/w photo)
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Dancers of the Opera Paris Ballet for USSR, here at Bourget airport, Paris, December 26, 1969 : Claire Motte, Claude Bessy, Jean-Pierre Bonnefous, Jacqueline Rayet, Yvette Chauvire, Josette Amiel (b/w photo)
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George Balanchine (1904-1983) Russian Choreographer and Ballet Master during Rehearsal For Ballet "Bourree Fantasque" With Dancer Jacqueline Rayet at Paris Opera House December 17, 1963 (b/w photo)
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Dancers of the Paris Opera are going to leave Paris for Montreal, here at Orly airport, July 23, 1967 : Martine Parmain, Jacqueline rayet, Michel Descombey, Yvette Chauvire, Claude Bessy, Claire Motte (b/w photo)
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Dancers of the Paris Opera leaving Paris for Montreal, here at Orly airport, July 23, 1967 : Yvette Chauvire, Jacqueline Rayet, Claude Bessy, Cyril Atanassof, Attilio Labis, Jean Pierre Bonnefous and Claire Motte (b/w photo)
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At The Premiere Of The Festival International De Danse De Paris Mrs. Claude Pompidou (Right) Conversing With The Dancer Star Of The Opera De Paris Jacqueline Rayet Sous Le Regard By Mr Michel Guy At The Theatre Des Champs Elysees November 3, 1967 Neg: C73616 (b/w photo)
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