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    61. Main Sequence Stars
    ... where n is about 4 for Sun-like stars, 3 for the more massive stars and 2.5 for dim red main sequence stars. ... A 0.1 solar mass star has only about one-thousandth the luminosity of the Sun whereas a 10-solar mass star is has a luminosity ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/outreach/education/senior/astrophysics/stellarevolution_mainsequence.html -- 75.1 Кб -- 11.04.2016
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    62. http://www.atnf.csiro.au/research/conferences/Parkes50th/ProcPapers/ellingsen.pdf
    ... style emulateapj v. 11/10/09 AN EVOLUTIONARY TIMELINE FOR HIGH-MASS STAR FORMATION S ... the physical process through which high-mass stars form remains nearly as much of a ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/conferences/Parkes50th/ProcPapers/ellingsen.pdf -- 348.3 Кб -- 08.10.2012
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    63. Structures of the Interstellar Medium in the LMC
    ... The structure of the ISM is determined by the interplay between massive stars and the ISM: molecular clouds form massive stars; massive stars dissociate, ionize, and dynamically structure the ambient medium; the ionized medium eventually cools, recombines ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/chu/paper/node3.html -- 60.7 Кб -- 08.04.2016
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    64. ATNF Colloquium
    ... Rosie Chen . Spitzer's View of Massive Star Formation in the Magellanic System - Rosie Chen Colloquium. ... providing an excellent opportunity to study massive star formation at . ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/news.php?action=show_item&item_id=748 -- 27.4 Кб -- 01.03.2014
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    65. http://www.atnf.csiro.au/pub/people/jreynold/joint97/joint97.lis
    ... Scientific Results ================== 3-D modelling of the Jovian radiation belts I de Pater (UC Berkeley) Mass outflows from extremely massive stars J.Chapman (ATNF) Exploring massive star formation through methanol and OH maser studies. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pub/people/jreynold/joint97/joint97.lis -- 2.3 Кб -- 24.02.1997
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    66. http://www.atnf.csiro.au/research/hypercompact/talks/Hill.pdf
    ... file v2.2) Physical characterisation of southern massive star-forming regions using Parkes NH3 observations arXiv:0911.4479v1 ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/hypercompact/talks/Hill.pdf -- 1700.0 Кб -- 07.09.2010
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    67. Binary and Variable Stars
    ... have allowed astronomers to determine the masses of stars and provided a wealth of ... explain the importance of binary stars in determining stellar masses . ... Binary Types . Masses of Stars . Binary Simulation . Types of Variable Stars . ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/outreach/education/senior/astrophysics/binary_variabletop.html -- 52.5 Кб -- 11.04.2016
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    68. CASS News
    ... in the Universe - are produced when massive stars explode and their cores collapse ... although evidence has been building since 1997 that massive stars are the culprits ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/news.php?action=show_item&item_id=337 -- 26.2 Кб -- 01.03.2014
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    69. http://www.atnf.csiro.au/research/workshops/2013/astroinformatics/talks/Lumsden-astroinformatics2013.pdf
    ... James Urquhart, Hugh Wheelwright (MPIfR), Joe Mottram (Leiden), Ben Davies, Toby Moore (Liverpool JMU), Cormac Purcell (Sydney), Michael Burton (UNSW) The RMS Survey ­ Finding the Galaxy's Young Massive Stars Solving the problem of how massive stars form ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/workshops/2013/astroinformatics/talks/Lumsden-astroinformatics2013.pdf -- 1642.7 Кб -- 11.12.2013
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    70. http://www.atnf.csiro.au/pasa/15_1/wyse/paper.pdf
    ... of present-day/recent massive-star formation is traced by H emission, while the past ... The variation of massive-star formation in NGC 6946 as inferred from the H ... H emission when estimating the massive-star formation rate can Star Formation in ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/wyse/paper.pdf -- 314.2 Кб -- 14.05.1998
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