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    21. Parkes_report
    ... After Stars" follows a red supergiant that is about to explode and considers whether it will produce a black hole or a pulsar. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/newsletter/feb05/Parkes_report.htm -- 11.1 Кб -- 23.01.2013
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    22. IAU Symposium 242
    ... Richards . Anita . Jodrell Bank Observatory . The story of red supergiant winds written in water . pdf (1.5 MB) . Yes . No . ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/masermeeting/web_papers/papers.html -- 91.3 Кб -- 28.02.2014
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    23. http://www.atnf.csiro.au/management/atuc/2006jun/docs/4_Astrophys.pdf
    ... The presence o f NH3 around Car hints that molecular shells around some Wolf-Rayet stars could have originated in prior LBV eruptions, rather than in cool red supergiant winds or the ambient interstellar medium. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/management/atuc/2006jun/docs/4_Astrophys.pdf -- 1379.3 Кб -- 02.06.2006
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    24. http://www.atnf.csiro.au/people/bkoribal/stars/HD93129.ps
    ... According to Crowther et al. (1995), the most massive (> 60 M ) O stars evolve from the Of stage directly into highly luminous late WN(+abs) and WN7 stars without passing through an intermediate Luminous Blue Variable or red supergiant phase. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/bkoribal/stars/HD93129.ps -- 330.4 Кб -- 01.12.2003
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    25. http://www.atnf.csiro.au/news/newsletter/feb07/ATNFnews_07Feb.pdf
    ... Smith on similar structures around Luminous Blue Variable stars in our own Galaxy calling into question the usual evolutionary scenario which invokes a transition of the progenitor of SN1987A from a red supergiant to a blue supergiant in the recent past ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/news/newsletter/feb07/ATNFnews_07Feb.pdf -- 2294.9 Кб -- 13.04.2007
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    26. http://www.atnf.csiro.au/news/newsletter/feb07/ATNFnews_07Feb_lowres.pdf
    ... Smith on similar structures around Luminous Blue Variable stars in our own Galaxy calling into question the usual evolutionary scenario which invokes a transition of the progenitor of SN1987A from a red supergiant to a blue supergiant in the recent past ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/news/newsletter/feb07/ATNFnews_07Feb_lowres.pdf -- 801.3 Кб -- 13.04.2007
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    27. http://www.atnf.csiro.au/pasa/17_2/bessell/paper.pdf
    ... Note the blue main sequence stars Be stars (pink), red supergiants (orange); A supergiant (white) The largest cluster of young massive stars in the SMC The beautiful h Car nebula. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/pasa/17_2/bessell/paper.pdf -- 73.9 Кб -- 15.09.2000
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    28. http://www.atnf.csiro.au/news/newsletter/apr09/ATNFnews_Apr09_lowres.pdf
    ... 2007; Pastorello et al. 2007] or changed from a slow to fast wind state such that it formed a wind-blown bubble (e.g., from a red supergiant to a Wolf-Rayet star ~50 ­ 100 years prior to SN; Weaver et al. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/news/newsletter/apr09/ATNFnews_Apr09_lowres.pdf -- 1067.2 Кб -- 16.06.2009
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    29. http://www.atnf.csiro.au/whats_on/workshops/mm_science2001/talks/Rudnitskij.pdf
    ... Millimetre Science with the Upgraded Australia Telescope 1 Late- type Variables · Red giant stars, M ~ 1 to a few M¤, L ~ a few ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/whats_on/workshops/mm_science2001/talks/Rudnitskij.pdf -- 500.7 Кб -- 23.04.2002
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    30. ASTRONOMERS FIND MOST MASSIVE COMPANION TO RADIO PULSAR
    ... it may be a massive late-type (red) star, a massive but compact blue star, or ... This turned up a bright, late-type (red) star with a K-band magnitude of 10.05 that ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/pulsar/pmsurv/press/1740_aas_pr.html -- 9.8 Кб -- 25.12.2007
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