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    31. THE AUSTRALIAN NATIONAL UNIVERSITY
    ... have detected 37 galaxies and one quasar in the string, but it probably contains many thousands of galaxies," Dr Francis said ... But in the early Universe, most galaxies had not yet formed, and most dark matter clouds will not yet contain a galaxy. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/string/ausrelease.htm -- 5.8 Кб -- 06.01.2004
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    32. http://www.mso.anu.edu.au/seminars/abstracts/20150602-1100.html
    ... Finally, I will present new dynamical scaling laws that link the baryonic mass distribution of a galaxy to the detailed shape of its rotation curve: these relations can be thought of as local inner-galaxy counterparts of the BTFR. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150602-1100.html -- 4.5 Кб -- 10.04.2016
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    33. Philip Lah's Talks
    ... The HI gas content of galaxies around Abell 370,a galaxy cluster at z = 0.37" . ... Talk at 'Galaxy Metabolism: Galaxy Evolution Near and Far' conference . ... Exploring the Stellar Populations of Early-Type Galaxies in the 6dF Galaxy Survey" . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~plah/Home_Page_Stuff/talks.html -- 11.6 Кб -- 10.04.2016
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    34. http://www.mso.anu.edu.au/seminars/abstracts/20160218-1100.html
    ... on the AAT is currently taking integral field spectroscopy of ~3000 nearby galaxies as part of the SAMI Galaxy Survey ... galaxies, I will discuss the relationship between dynamical misalignments and the influence of environment, morphology and ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20160218-1100.html -- 4.7 Кб -- 10.04.2016
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    35. Research Interests
    ... For example, the division of stars in our galaxy into dynamically and chemically different populations (the thin and thick disks, halo and bulge) is surely telling us something crucial about how our galaxy formed. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight/node33.html -- 5.0 Кб -- 02.10.2012
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    36. Research Interests
    ... we look at the amount of gas as a function of redshift, it should drop as galaxies form, telling us the era of galaxy formation ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight/node9.html -- 5.2 Кб -- 02.10.2012
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    37. http://www.mso.anu.edu.au/seminars/abstracts/20150417-1420.html
    ... The SAMI Galaxy Survey has now observed more than a thousand galaxies from the nearby universe. ... Galaxy Survey data and discuss some of the work being done by RSAA on the emission line properties, in particular the ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150417-1420.html -- 4.0 Кб -- 10.04.2016
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    38. http://www.mso.anu.edu.au/~plah/Home_Page_Stuff/files/questacon_2011.pdf
    ... cm Emission From Galaxies Galaxy M33: optical Galaxy M33: HI 21-cm emission Galaxy M33: optical and HI Galaxy M33: optical Why ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~plah/Home_Page_Stuff/files/questacon_2011.pdf -- 2383.4 Кб -- 19.05.2011
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    39. http://www.mso.anu.edu.au/seminars/abstracts/20151210-1100.html
    ... Within galaxies, feedback regulates the structure of the interstellar medium, and many observed properties of the ISM, star formation, and galaxies can be understood as a fundamental consequence of super-sonic turbulence in a rapidly cooling, self ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151210-1100.html -- 5.3 Кб -- 10.04.2016
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    40. http://www.mso.anu.edu.au/pfrancis/roleplay/ziggy/model_answer2.pdf
    ... Ziggy seems to be located in the outer regions of an elliptical galaxy, or perhaps in a globular cluster orbiting such a galaxy ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/ziggy/model_answer2.pdf -- 50.6 Кб -- 12.06.2002
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