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    1. http://www.atnf.csiro.au/research/LVmeeting/magsys_pres/gaensler_sn1987a.pdf
    ... Kesteven, Lewis Ball, Tasso Tzioumis (ATNF) © Anglo-Australian Observatory / David Malin Images Circumstellar Structure · Dense slow red supergiant wind, concentrated into equatorial plane · High-velocity low-density isotropic blue supergiant wind for ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/LVmeeting/magsys_pres/gaensler_sn1987a.pdf -- 1069.1 Кб -- 29.07.2007
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    2. http://www.atnf.csiro.au/research/masermeeting/web_papers/503_RHumphreys.pdf
    ... circumstellar ejecta point sources: µ Cep Cas HR5171a HR8752 extended sources + complex ejecta VX Sgr S Per IRC +10420 NML Cyg VY CMa The Post Red Supergiant -- IRC +10420 Strong IR excess L ~ 5 x 105 Lsun High mass loss rate 3-6 x 10-4 One of warmest ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/masermeeting/web_papers/503_RHumphreys.pdf -- 697.0 Кб -- 09.04.2007
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    3. Post-Main Sequence Stars
    ... Credit: NASA . An artist's impression of a red supergiant engulfing a Jupiter-like planet as it expands. ... Credit: Andrea Dupree (Harvard-Smithsonian CfA), Ronald Gilliland ( STScI ), NASA and ESA . Betelgeuse is a red supergiant. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/outreach/education/senior/astrophysics/stellarevolution_postmain.html -- 67.1 Кб -- 11.04.2016
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    4. Questions on Stars
    ... in order of increasing luminosity: blue supergiant, the Sun, red giant, white dwarf ... from dimmest to most luminous would be: white dwarf, Sun, red giant, blue supergiant ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/outreach/education/senior/cosmicengine/stars_questions.html -- 51.7 Кб -- 11.04.2016
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    5. http://www.atnf.csiro.au/research/conferences/Parkes50th/ProcPapers/vanLoon.pdf
    ... long pulsation period: IRAS 05280-6910 is a red supergiant evolved from a 19-M main ... extremely luminous and late-type dusty red supergiant IRAS 04553-6825 (WOH G064; cf ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/conferences/Parkes50th/ProcPapers/vanLoon.pdf -- 277.4 Кб -- 02.10.2012
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    6. No Title
    ... in this line, which has a frequency near 658 GHz, toward a diverse sample of oxygen-rich red giant and supergiant stars ... The wavenumbers were determined from observations of the planetary nebula NGC 7027 and of the red supergiant Scorpii. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/plintel/groups/lsse/agb/950901/950901.html -- 76.2 Кб -- 12.04.2016
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    7. No Title
    ... The transition of a massive post-main sequence star from red supergiant to luminous blue variable or Wolf-Rayet star is a rapid ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/plintel/groups/lsse/agb/950501/950501.html -- 90.0 Кб -- 12.04.2016
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    8. Photometry Questions
    ... If we also know its luminosity class we can further constrain its position along this line, that is we can distinguish between a red supergiant, giant or main sequence star for example. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/outreach/education/senior/astrophysics/photometry_questions.html -- 66.6 Кб -- 11.04.2016
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    9. http://www.atnf.csiro.au/research/masermeeting/web_papers/505_Richards.pdf
    ... Story of Red Supergiant Winds written in water A.M.S.Richards, I.Bains, A.Bartkiewicz, R.J.Cohen, P.J.Diamond, S.Etoka, M.D.Gray, E.E.Lekht, E.Mendoza-Torres, M.R.W.Masheder, K.Murakawa, M.Szymczak, H.J.van Langevelde, W.Vlemmings, J.A.Yates High-mass AGB ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/masermeeting/web_papers/505_Richards.pdf -- 1536.0 Кб -- 13.03.2007
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    10. Spectroscopic Parallax
    ... If we also know its luminosity class we can further constrain its position along this line, that is we can distinguish between a red supergiant, giant or main sequence star for example. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/outreach/education/senior/astrophysics/photometry_specparallax.html -- 53.2 Кб -- 11.04.2016
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