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    21. http://www.mso.anu.edu.au/~gdc/talks/LocalGroupLect_17Dec2012.pdf
    ... Components: · 2 large spiral (disk) galaxies the Milky Way, and Andromeda (M31) M31 is somewhat larger and more luminous than the Milky Way: MV (M31) ~ -21.1 while MV (MWG) ~ -20.6 (MV = -20.6 corresponds to 1.4 x 10 10 L sun) M31 and the Milky Way ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~gdc/talks/LocalGroupLect_17Dec2012.pdf -- 2242.9 Кб -- 17.12.2012
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    22. http://www.mso.anu.edu.au/~gdc/talks/LocalGroupWinterSchols.pdf
    ... Components: · 2 large spiral (disk) galaxies the Milky Way, and Andromeda (M31) M31 is somewhat larger and more luminous than the Milky Way: MV (M31) ~ -21.1 while MV (MWG) ~ -20.6 (MV = -20.6 corresponds to 1.4 x 10 10 L sun) M31 and the Milky Way ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~gdc/talks/LocalGroupWinterSchols.pdf -- 2231.9 Кб -- 28.06.2011
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    23. http://www.mso.anu.edu.au/~gdc/talks/LocalGroupLect_Dec2014.pdf
    ... Components: · 2 large spiral (disk) galaxies the Milky Way, and Andromeda (M31) M31 is somewhat larger and more luminous than the Milky Way: MV (M31) ~ -21.1 while MV (MWG) ~ -20.6 (MV = -20.6 corresponds to 1.4 x 10 10 L sun) M31 and the Milky Way ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~gdc/talks/LocalGroupLect_Dec2014.pdf -- 2249.6 Кб -- 08.12.2014
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    24. http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Fuchs02
    ... The selected galaxies show all clear spiral structure and arguments of density wave ... For this purp ose galaxies were selected which show clear spiral structure. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Fuchs02 -- 78.4 Кб -- 09.07.2007
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    25. http://www.mso.anu.edu.au/~kcf/surya/bars/Palunas00
    ... in U.S.A. MAXIMUM DISK MASS MODELS FOR SPIRAL GALAXIES POVILAS PALUNAS1,2 Laboratory for Astronomy and Solar Physics, NASA ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/bars/Palunas00 -- 2026.1 Кб -- 09.07.2007
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    26. http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Fuchs02a
    ... An LSBG is usually defined as a spiral galaxy with a central surface brightness 1 ... If, for example, a galaxy shows clear spiral structure, arguments from density wave ... All selected galaxies show two­armed spiral structure (m = 2). Table 1. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Fuchs02a -- 191.9 Кб -- 13.07.2007
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    27. http://www.mso.anu.edu.au/~kcf/surya/misc_papers/McGaugh07
    ... dark matter -- galaxies: kinematics and dynamics -- galaxies: spiral arXiv:astro-ph ... Introduction The rotation curves of spiral galaxies provide one of the strongest ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~kcf/surya/misc_papers/McGaugh07 -- 619.1 Кб -- 14.12.2006
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    28. COALA - Computational Astrophysics Laboratory
    ... problem (Steinmetz Navarro 1999); the number and sizes of spiral galaxies in simulations are smaller than those observed, and ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/coala/universe.html -- 4.8 Кб -- 01.10.2012
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    29. Research Interests
    ... What are these galaxies? You hypothesise that they are the ancestors of the bulges of normal spiral galaxies today. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight/node12.html -- 5.6 Кб -- 02.10.2012
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    30. Research Interests
    ... Galaxy clusters have also changed: at redshifts around one, clusters seem to contain more spiral galaxies, fewer S0s and the same number of giant elliptical galaxies as we see today. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight/node6.html -- 5.3 Кб -- 02.10.2012
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