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    • [ В начало ] Пред. | 11 | 12 | 13 | 14 | 15 | 16 | 17 | 18 | 19 | 20 | След.

    141. http://www.mso.anu.edu.au/~brian/publications.pdf
    ... Wyithe, J. Stuart B., Loeb, Abraham, Schmidt, Brian P., 2007, MNRAS, 380, 1087 "The correlation between star formation and 21-cm emission during the reionization epoch" 21. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~brian/publications.pdf -- 91.5 Кб -- 13.12.2010
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    142. http://www.mso.anu.edu.au/~geoff/Papers/Rad_Shock_1.pdf
    ... established research area in astrophysics and the insight gained by numerical simulations has advanced our knowledge in many topics including astrophysical jets, accretion discs, cosmology, star formation, supernovae and stellar structure, to name a few ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/Papers/Rad_Shock_1.pdf -- 265.1 Кб -- 21.06.2002
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    143. http://www.mso.anu.edu.au/seminars/abstracts/20150205-1100.html
    ... to the formation and evolution of our Galaxy, the Milky Way, are hidden in the chemical abundances and kinematics of its stars ... However, stars that were accreted during the earliest times of the formation of the Galactic halo have been elusive. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150205-1100.html -- 6.1 Кб -- 10.04.2016
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    144. http://www.mso.anu.edu.au/~kcf/surya/Sellwood.Deb06.pdf
    ... Barred galaxies having gas and on-going star formation would be expected to have stronger spirals. 7.2. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/Sellwood.Deb06.pdf -- 432.4 Кб -- 31.07.2007
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    145. http://www.mso.anu.edu.au/~kcf/surya/swaters00
    ... If these high values of U are to be explained solely by a stellar population, the stellar content and the processes of star formation in LSB galaxies need to be ver y different from those in HSB galaxies. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/swaters00 -- 112.4 Кб -- 31.07.2007
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    146. http://www.mso.anu.edu.au/~charley/papers/GretherLineweaver06.pdf
    ... INTRODUCTION The formation of a binary star via molecular cloud fragmentation and ... have been suggested for the formation of companion stars, brown dwarfs, and planets ... to Sun-like stars to help constrain their formation and migration scenarios ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/GretherLineweaver06.pdf -- 1342.2 Кб -- 10.05.2006
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    147. http://www.mso.anu.edu.au/~kcf/surya/misc_papers/McGaugh07
    ... Perhaps the most common example is feedback from star formation. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/misc_papers/McGaugh07 -- 619.1 Кб -- 14.12.2006
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    148. http://www.mso.anu.edu.au/~kcf/pubs_top20/100.pdf
    ... If we assume that this increased rate of SN Ia production is related to the higher rate of star formation in spirals, then the SNe Ia in spirals come from progenitors that are likely to be younger than the progenitors of SNe Ia in ellipticals. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/100.pdf -- 1358.4 Кб -- 16.10.2011
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    149. http://www.mso.anu.edu.au/~raquel/thesis-final.pdf
    ... Magnetic fields and star formation: theory versus observations, eds. A. I. Gomez de ... ortant roles in the dynamics of star formation and, in particular, in the evolution ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~raquel/thesis-final.pdf -- 2716.5 Кб -- 21.11.2006
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    150. http://www.mso.anu.edu.au/seminars/abstracts/20151120-1420.html
    ... Eloise Birchall . "Masters Thesis Proposal: Signs of Planet Formation in Disks Around Young High-Intermediate Mass Stars". ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151120-1420.html -- 4.0 Кб -- 10.04.2016
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