File:Wolf rayet2.jpg
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描述Wolf rayet2.jpg |
This NASA Hubble Space Telescope picture of the energetic star WR124 reveals it is surrounded by hot clumps of gas being ejected into space at speeds of over 100,000 miles per hour. Also remarkable are vast arcs of glowing gas around the star, which are resolved into filamentary, chaotic substructures, yet with no overall global shell structure. Though the existence of clumps in the winds of hot stars has been deduced through spectroscopic observations of their inner winds, Hubble resolves them directly in the nebula M1-67 around WR124 as 100 billion-mile wide glowing gas blobs. Each blob is about 30 times the mass of the Earth. The massive, hot central star is known as a Wolf-Rayet star. This extremely rare and short-lived class of super-hot star (in this case 50,000 degrees Kelvin) is going through a violent, transitional phase characterized by the fierce ejection of mass. The blobs may result from the furious stellar wind that does not flow smoothly into space but has instabilities which make it clumpy. The surrounding nebula is estimated to be no older than 10,000 years, which means that it is so young it has not yet slammed into the gasses comprising the surrounding interstellar medium. The star is 15,000 light-years away, located in the constellation Sagitta. The picture was taken with Hubble's Wide Field Planetary Camera 2 in March 1997. The image is false-colored to reveal details in the nebula's structure. |
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来源 | http://hubblesite.org/newscenter/archive/releases/1998/38/image/a/ (direct link) | ||||
作者 | Yves Grosdidier (University of Montreal and Observatoire de Strasbourg), Anthony Moffat (Universitie de Montreal), Gilles Joncas (Universite Laval), Agnes Acker (Observatoire de Strasbourg), and NASA | ||||
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日期/时间 | 缩略图 | 大小 | 用户 | 备注 | |
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当前 | 2010年2月1日 (一) 10:05 | 611 × 641(606 KB) | Tryphon(留言 | 贡献) | Original size, from http://hubblesite.org/newscenter/archive/releases/1998/38/image/a/. | |
2008年10月18日 (六) 12:36 | 1,122 × 1,179(349 KB) | Henrykus(留言 | 贡献) | {{Information |Description= HST image of Wolf-Rayet star WR 124 surrounded by M1-67 nebula. |Source= http://rst.gsfc.nasa.gov/Sect20/A6.html description from http://heasarc.gsfc.nasa.gov/docs/objects/heapow/archive/transients/march03_grbs.html |Date= |Au | ||
2005年8月27日 (六) 14:08 | 360 × 378(70 KB) | Joonasl(留言 | 贡献) | HST image of a Wolf-Rayet star {{PD-USGov-NASA}} Category:astronomy |
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