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    131. http://www.mso.anu.edu.au/pfrancis/papers/2126-158.ps
    ... are observed to be ellipticals: each shows a passive elliptical galaxy spectrum, and none shows evidence for on­going star­formation (for instance, through the presence of an [O ii] emission line), which would indicate the presence of large amounts of gas ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/papers/2126-158.ps -- 2216.3 Кб -- 15.02.2006
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    132. http://www.mso.anu.edu.au/~kcf/pubs_top20/25.pdf
    ... et al. (1996) and Riess et al. (1999) show that the most luminous SNe Ia occur only in galaxies with ongoing star formation ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/25.pdf -- 888.8 Кб -- 16.10.2011
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    133. http://www.mso.anu.edu.au/~kcf/surya/misc_papers/McGaugh05
    ... Above this color, one expects variation in to settle down, as the effects of individual star formation events are moderated by the accumulation of mass from previous generations. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/misc_papers/McGaugh05 -- 451.7 Кб -- 26.09.2006
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    134. http://www.mso.anu.edu.au/seminars/abstracts/20141204-1100.html
    ... Our theoretical and observational work makes us increasingly confident, however, that the Bubbles were inflated, over much longer timescales, by the intense star-formation occurring around the SMBH. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20141204-1100.html -- 5.2 Кб -- 10.04.2016
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    135. http://www.mso.anu.edu.au/~chiaki/works/TEN80301.pdf
    ... To clarify the underlying physical processes from such observational data, we simulate the chemodynamical evolution of galaxies including star formation, supernovae, and chemical enrichment. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~chiaki/works/TEN80301.pdf -- 2146.0 Кб -- 08.02.2008
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    136. http://www.mso.anu.edu.au/~fbriggs/LOFAR_SciApp_1.0.pdf
    ... distant objects, providing important constraints upon early star formation epochs ... density, relates directly to the instantaneous star-formation rate in these systems ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~fbriggs/LOFAR_SciApp_1.0.pdf -- 1914.3 Кб -- 17.04.2003
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    137. http://www.mso.anu.edu.au/pfrancis/roleplay/newstarform.pdf
    ... Star and Planet Formation Role-Playing Exercise Paul Francis Original Version April 1997. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/newstarform.pdf -- 58.2 Кб -- 15.04.2004
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    138. http://www.mso.anu.edu.au/~charley/papers/LineweaverEgan2008v2.pdf
    ... The efficiency of star formation in a molecular cloud is a few percent. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/LineweaverEgan2008v2.pdf -- 826.4 Кб -- 18.03.2009
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    139. http://www.mso.anu.edu.au/pfrancis/comets/comets.pdf
    ... If most stars have planets, and if planetary formation is usually accompanied by comet ejection, then there should be a ... Series. 323, Star Formation in the Interstellar Medium, Ed. D. Johnstone et al., 371 Dohnanyi, J.S., 1969, J. Geophys. Res., ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/comets/comets.pdf -- 1827.0 Кб -- 06.09.2005
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    140. http://www.mso.anu.edu.au/annualReport/1999/annualrep1999.pdf
    ... excited by stars of a wide variety of ages, in a region of continuous star formation ... Galactic Nuclei (AGN), while in others the infrared source is intense star formation ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/annualReport/1999/annualrep1999.pdf -- 1204.9 Кб -- 15.10.2004
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