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    131. http://www.mso.anu.edu.au/pfrancis/roleplay/newstarform.pdf
    ... This black hole will attract other black holes, and over a period of 1011 years will swallow any nearby black holes and stars, getting more and more massive as it does so. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/newstarform.pdf -- 58.2 Кб -- 15.04.2004
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    132. http://www.mso.anu.edu.au/seminars/abstracts/20141118-1100.html
    ... High resolution spectroscopy for many RGB stars in dwarf galaxies over a range of masses show how each has had a unique chemical evolution. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20141118-1100.html -- 4.3 Кб -- 10.04.2016
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    133. http://www.mso.anu.edu.au/~chiaki/works/TEN80301.pdf
    ... Stars in present-day massive galaxies formed in smaller galaxies at high redshifts, despite their late assembly times. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~chiaki/works/TEN80301.pdf -- 2146.0 Кб -- 08.02.2008
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    134. http://www.mso.anu.edu.au/~kcf/ATA/pan_spectr.pdf
    ... This limit defines a horizon out to which we can work: for dwarf stars, this corresp onds to a distance of ab out 3 kp c. Out to this horizon, the mass of thick disk stars is ab out 2 в 109 M . ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/ATA/pan_spectr.pdf -- 76.8 Кб -- 12.08.2008
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    135. http://www.mso.anu.edu.au/~kcf/pubs_top20/101.pdf
    ... 1998). Younger white dwarfs are expected to evolve from more massive stars with a lower ratio of C/O in their cores. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/101.pdf -- 2259.2 Кб -- 16.10.2011
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    136. http://www.mso.anu.edu.au/~kcf/surya/misc_papers/Conselice05
    ... the fraction of total mass that has condensed into stars is distributed with both ... masses and stellar masses of disk galaxies should correlate if star formation is ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/misc_papers/Conselice05 -- 240.6 Кб -- 19.12.2006
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    137. http://www.mso.anu.edu.au/~kcf/pubs_top20/25.pdf
    ... 332, The Fate of the Most Massive Stars, ed. R. Humphreys & K. Stanek (San Francisco: ASP), 33 ------. 2005b, in White Dwarfs: Cosmological and Galactic Probes, ed. E. M. Sion, S. Vennes, & H. L. Shipman ( Dordrecht: Springer), 97 Filippenko, A. V., Li, W ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/25.pdf -- 888.8 Кб -- 16.10.2011
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    138. http://www.mso.anu.edu.au/seminars/abstracts/20151209-1100.html
    ... Since the collision time scale is short ~10^5 yrs, O star formation is a rapid process with a mass accretion rate higher than 10^-4Mo/yr.. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151209-1100.html -- 4.3 Кб -- 10.04.2016
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    139. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/aa_paper_on_spectrophotometry.pdf
    ... to observe a series of "" smooth оо spectrum stars during the 1431 night at air masses encompassing those for the program stars ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/aa_paper_on_spectrophotometry.pdf -- 231.5 Кб -- 29.11.2004
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    140. http://www.mso.anu.edu.au/~bessell/bescast.pdf
    ... the model colors for different abundances, luminosities and masses should enable equally as reliable temperatures to be derived for stars of all mass and age (for very extreme cases, like very metalpoor stars more tests will be needed as different opacity ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~bessell/bescast.pdf -- 412.6 Кб -- 09.04.2006
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