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    31. Untitled1
    ... masses near that of the sun and young stars with masses up to 100 times the sun's ... Cepheids are relatively massive stars (3-5 times the mass of the Sun) that regularly ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/annualReport/1997/07_research.html -- 73.5 Кб -- 02.10.2012
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    32. http://www.mso.anu.edu.au/~charley/papers/0412356.pdf
    ... preferentially find planets around lower mass stars where a greater radial velocity ... Hence again finding planets around the lower mass stars (early K sp ectral typ e) in ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/0412356.pdf -- 1446.8 Кб -- 15.12.2004
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    33. http://www.mso.anu.edu.au/~charley/papers/EganLineweaverApJOnline.pdf
    ... yellow fill in the top panel represents stars of mass 1M M 8 M , which died leaving ... The blue fill represents stars of mass 8 M M 25 M , which died and left neutron star ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/EganLineweaverApJOnline.pdf -- 1187.8 Кб -- 04.02.2010
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    34. Dougal Mackey - Research
    ... driven galaxy formation and mass assembly across cosmological history via the resolved (star-by-star) study of nearby systems ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~dougal/research.html -- 8.7 Кб -- 09.04.2016
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    35. http://www.mso.anu.edu.au/~charley/papers/Icarus.pdf
    ... If low mass star formation is suppressed in low metallicity molecular clouds (Nishi ... Way disk (Favata et al. 1997), of massive OB stars (Gummersbach et al. 1998), and of ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/Icarus.pdf -- 159.7 Кб -- 17.05.2002
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    36. Supernovae
    ... is a sub-category of cataclysmic variable stars that results from the internal collapse and violent explosion of a massive star ... Stars must have at least 9 times the mass of the Sun in order to undergo a core-collapse. METHOD . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~jerjen/researchprojects/sn/sn.html -- 8.2 Кб -- 02.10.2012
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    37. http://www.mso.anu.edu.au/~charley/papers/0909.3983v1.pdf
    ... fill in the top panel represents stars of mass 1M < M < 8M , which died leaving ... Th e blue fill represents stars of mass 8M < M < 25M , which died and left neutron ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/0909.3983v1.pdf -- 929.8 Кб -- 25.09.2009
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    38. Home Page of Raquel Salmeron
    ... Spinning discs in space Mass feeding and feedback in YSOs . ScienceAlert Ever wonder how solar-mass stars form? . By Tim Wetherell. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~raquel/ -- 6.6 Кб -- 01.10.2012
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    39. RSAA Seminars - Intranet - ANU
    ... Signs of Planet Formation in Disks Around Young High-Intermediate Mass Stars ... Discovering and characterising transiting planets and low mass stars . ... Very Massive Stars . 31/03/2015, 11:00-12:00 . Duffield Lecture Theatre . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/past.php -- 76.8 Кб -- 09.04.2016
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    40. http://www.mso.anu.edu.au/~charley/papers/RoblesLineweaverAstroph.pdf
    ... For a main sequence star, mass determines luminosity, effective temp erature, main ... 1993). Low mass stars are intrinsically dim. ... to b e a proxy for the fraction of a star's mass that is not hydrogen or helium ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/RoblesLineweaverAstroph.pdf -- 2242.0 Кб -- 20.05.2008
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