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    • [ В начало ] Пред. | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 | 17 | 18 | След.

    121. http://www.mso.anu.edu.au/~gdc/talks/LocalGroupLect_Dec2013.pdf
    ... have high DARK MATTER content ­ in some dwarfs the mass/light ratio (with mass measured via the velocity dispersion of the stars or via the circular velocity of the gas) exceeds 100, while the mass-to-light ratio of the stars is typically of order unity ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~gdc/talks/LocalGroupLect_Dec2013.pdf -- 2249.0 Кб -- 11.12.2013
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    122. http://www.mso.anu.edu.au/~gdc/talks/LocalGroupWinterSchols.pdf
    ... have high DARK MATTER content ­ in some dwarfs the mass/light ratio (with mass measured via the velocity dispersion of the stars or via the circular velocity of the gas) exceeds 100, while the mass-to-light ratio of the stars is typically of order unity ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~gdc/talks/LocalGroupWinterSchols.pdf -- 2231.9 Кб -- 28.06.2011
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    123. http://www.mso.anu.edu.au/~charley/papers/Chapter22Lineweaver.pdf
    ... the masses of black holes 22.1 The Entropy of the Observable Universe Stars are ... nuclei, binary X-ray sources), star formation and even massive planet formation ... When an accretion disk around a star runs out of mass to accrete and is no longer ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/Chapter22Lineweaver.pdf -- 588.6 Кб -- 17.03.2014
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    124. http://www.mso.anu.edu.au/~gdc/talks/LocalGroupLect_Dec2014.pdf
    ... have high DARK MATTER content ­ in some dwarfs the mass/light ratio (with mass measured via the velocity dispersion of the stars or via the circular velocity of the gas) exceeds 100, while the mass-to-light ratio of the stars is typically of order unity ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~gdc/talks/LocalGroupLect_Dec2014.pdf -- 2249.6 Кб -- 08.12.2014
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    125. http://www.mso.anu.edu.au/~kcf/surya/misc_papers/Noordermeer07
    ... In the other cases, however, no strong nuclear activity is observed and the most natural explanation of the observed velocities is a nuclear disk or ring, p ossibly rotating around a massive nuclear star cluster or sup er-massive black hole. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/misc_papers/Noordermeer07 -- 654.2 Кб -- 25.01.2007
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    126. http://www.mso.anu.edu.au/~kcf/pubs_top20/34.pdf
    ... most likely within the Sco­Cen association, a massive region of star formation in the southern Milky Way (Zuckerman & Song 2004 ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/34.pdf -- 664.4 Кб -- 15.10.2011
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    127. http://www.mso.anu.edu.au/seminars/abstracts/20141120-1100.html
    ... In addition, several observed relationships, including cosmic star formation rate density, galaxy luminosity function, and [alpha/Fe]-mass, can only begin to be reproduced when it is included. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20141120-1100.html -- 4.3 Кб -- 10.04.2016
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    128. http://www.mso.anu.edu.au/seminars/abstracts/20150327-1420.html
    ... There is now strong evidence for stars that have been born with initial helium mass fractions as high as Y=0.40, such as in the globular cluster Omega Centauri. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150327-1420.html -- 4.2 Кб -- 10.04.2016
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    129. http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Fuchs02
    ... Mass estimates of the combined star and gas disks of the LSBGs are given in the fourth column. ... which might indicate that LSBGs with high mass­to­light ratios have consumed by star formation more of their interstellar gas ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Fuchs02 -- 78.4 Кб -- 09.07.2007
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    130. http://www.mso.anu.edu.au/~gdc/prepr/AndII_vars.pdf
    ... metal-poor stars or stars that have formed from mass-transfer in a binary system ... ACs are believed to be either stars that have increased mass due to mass transfer in ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~gdc/prepr/AndII_vars.pdf -- 889.2 Кб -- 05.11.2003
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