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    71. http://www.mso.anu.edu.au/~charley/papers/LineweaverDavis.pdf
    ... zones around these stars may be a common feature of star formation (Kasting et al ... is a common by-product of star formation and that the fraction of stars with ... formation is a common feature of star formation (Wetherill, 1996; Lissauer and Lin ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/LineweaverDavis.pdf -- 492.9 Кб -- 11.12.2004
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    72. Marc White - Astrophysicist - The Australian National University
    ... 2011 . Star Formation Through Spectroimaging at High Angular Resolution . Star Formation Summer School . Taipei, Taiwan . ... Star Formation Through Spectroimaging at High Angular Resolution . Star Formation Summer School . Taipei, Taiwan . 2011 . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~mwhite/CV.php -- 9.2 Кб -- 09.04.2016
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    73. COALA - Sharon Rapoport
    ... should help better define the progenitor systems that lead to bright GRBs, illuminate the range of physics that lead to bright GRBs, and allow us to better understand and predict the biases that are associated with using GRBs as tracers of star formation ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/coala/sharon.html -- 5.8 Кб -- 01.10.2012
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    74. Untitled1
    ... the MACHO Database: Constraints on the Star Formation Rate and on Stellar Models", D ... Caltech, colloquium: "The Star Formation History of Galaxies Near Us". ... Invited talk: "The Star Formation History of Galaxies studied with WFPC2". ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/annualReport/1997/11_staffAct.html -- 51.3 Кб -- 02.10.2012
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    75. http://www.mso.anu.edu.au/seminars/abstracts/20160315-1100.html
    ... Furthermore, such a single r-process event is a uniquely stringent constraint on the metal mixing and star formation history of this ultra-faint dwarf galaxy. (accepted for publication in Nature, http://arxiv.org/abs/1512.01558) . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20160315-1100.html -- 5.4 Кб -- 10.04.2016
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    76. RSAA Annual Report 1998
    ... in the MACHO database: Constraints on the star formation rate and on stellar models ... Jet-Induced Emission-Line Nebulosity and Star Formation in the High-Redshift Radio ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/annualReport/1998/13_publications.html -- 76.5 Кб -- 02.10.2012
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    77. http://www.mso.anu.edu.au/~bessell/publications1.txt
    ... sample of long-period variables in the bar of the LMC and evidence for a recent burst of star formation" ApJ 290, 477-486, 1985 ... Mould, J. et al. "Jet-induced Star Formation in Centaurus A", ApJ, 536, 266 163. Stathakis, R. A. et al. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~bessell/publications1.txt -- 27.0 Кб -- 06.12.2002
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    78. http://www.mso.anu.edu.au/seminars/abstracts/20151008-1100.html
    ... I will discuss how relative abundance measurements in this extremely metal-poor regime enable us to test models of Population III star formation, early gas enrichment and metal mixing. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151008-1100.html -- 4.7 Кб -- 10.04.2016
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    79. http://www.mso.anu.edu.au/~charley/papers/CosmicThermoBiology.pdf
    ... This initiated collapse and star formation. One of the stars was the Sun. ... of the hydrogen is low enough to initiate gravitational collapse and star formation ... billion years after the big bang) to the formation of the first stars and planets ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/CosmicThermoBiology.pdf -- 201.9 Кб -- 12.05.2003
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    80. http://www.mso.anu.edu.au/~geoff/AGD/Sound_Waves.pdf
    ... nebula is a dark molecular cloud that is the site of ongoing star formation ... Star formation - the modern approach The above discussion is the standard treatment ... mass is that the physics of star formation is more complicated and that magnetic ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/AGD/Sound_Waves.pdf -- 252.2 Кб -- 22.02.2016
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