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    21. http://www.mso.anu.edu.au/seminars/abstracts/20150804-1100.html
    ... Some astronomers ignore low-mass stars because they aren t very bright. ... However, stars with initial masses between about 0.8 Msun and 8 Msun (AGB stars) play an important role as the main site of the ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150804-1100.html -- 4.5 Кб -- 10.04.2016
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    22. http://www.mso.anu.edu.au/~charley/papers/isjupnew2.pdf
    ... observations of star-forming regions indicate that massive stars disrupt the protoplanetary disks around neighboring lower mass ... This value for is close to the ;0:8 0:2 found for very low mass stars (Bejar et al. 2001). ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/isjupnew2.pdf -- 252.8 Кб -- 07.08.2002
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    23. http://www.mso.anu.edu.au/annualReport/2002/RSAA_AnnRep_2002.pdf
    ... that a supernova (an exploding massive star) coincided with a cosmological gamma ray ... Telescope, which showed that the exploding object had to be a massive star ... is that GRBs occur when a massive star's core collapses into a black hole, which ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/annualReport/2002/RSAA_AnnRep_2002.pdf -- 1830.6 Кб -- 15.10.2004
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    24. http://www.mso.anu.edu.au/~kcf/pubs_top20/95.pdf
    ... the supernova are in contrast to what is expected for such massive stars and indicate that a new sort of explosion may have ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/95.pdf -- 160.2 Кб -- 16.10.2011
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    25. Cepheid Variables
    ... CEPHEID VARIABLE STARS: A Cepheid variable or Cepheid is a member of a particular class of very luminous, massive variable stars with pulsation periods of 1-70 days. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~jerjen/researchprojects/cepheids/cepheids.html -- 8.3 Кб -- 02.10.2012
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    26. http://www.mso.anu.edu.au/~geoff/HEA/HEA_overview.pdf
    ... M Solar Mass evolve to white dwarfs -> Planetary Nebulae · Higher mass stars evolve to Neutron stars or Black Holes -> Pulsars ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/HEA_overview.pdf -- 2636.4 Кб -- 04.03.2001
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    27. http://www.mso.anu.edu.au/seminars/abstracts/20151027-1100.html
    ... The spectra of AGN host galaxies contain emission lines excited by radiation from both massive stars and the AGN accretion disk. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151027-1100.html -- 4.8 Кб -- 10.04.2016
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    28. Research Interests
    ... These need massive black holes to power their activity, and it is hard to form black holes without forming stars and galaxies ... back down the potential wells until, Poof! it is all blown out again, leaving a few more neutron stars and low mass stars ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight/node30.html -- 6.1 Кб -- 02.10.2012
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    29. Dougal Mackey - Conference Proceedings
    ... Cambridge University Press, Cambridge, p. 275 . 9. Multiple stellar populations in massive LMC star clusters . ... Cambridge University Press, Cambridge, p. 273 . 4. Black holes and core expansion in massive star clusters . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~dougal/conference.html -- 10.8 Кб -- 09.04.2016
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    30. http://www.mso.anu.edu.au/~charley/papers/GretherLineweaver06.pdf
    ... Subject headingg stars: low-mass, brown dwarfs s: Online material: machine-readable ... preferentially find planets around lower mass stars where a greater radial velocity ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/GretherLineweaver06.pdf -- 1342.2 Кб -- 10.05.2006
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