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    11. http://www.mrao.cam.ac.uk/yerac/reynaud/reynaud.ps
    ... synthesis of a barred spiral By D. R e yn a ud & D. D o wn e s e­mail: reynaud@iraux2.iram.fr Institut de Radio Astronomie Millim'etrique, Grenoble, FRANCE NGC 1530 is one of the largest barred spiral galaxies in the northern sky, with bright CO emission ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/yerac/reynaud/reynaud.ps -- 407.8 Кб -- 22.02.1995
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    12. http://www.mrao.cam.ac.uk/projects/skads/lofar/talks/Beck.MKSP.Cambridge.pdf
    ... MKSP: Targets: Galactic sources: polarised Galactic regions (Fan, NPS); SNR, HII & planetary nebulae as Faraday screens Nearby galaxies: spiral, barred, edge-on, dwarf, interacting, blue compact, Virgo cluster members Intergalactic filaments, e.g. in ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/skads/lofar/talks/Beck.MKSP.Cambridge.pdf -- 2669.6 Кб -- 07.04.2009
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    13. http://www.mrao.cam.ac.uk/galevol/talk_abstracts.pdf
    ... Title: The Evolution of Spiral Galaxies in the Group Environment Abstract: Although ... environment on starformation rates (SFRs) of spiral galaxies in the lo cal Universe ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/galevol/talk_abstracts.pdf -- 226.0 Кб -- 29.08.2013
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    14. Scaling relations for molecular gas in the Large Magellanic Cloud
    ... The proximity of the LMC enables detailed studies of the molecular gas in an environment differing from that in quiescent spiral galaxies such as the Milky Way. ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/heikkilae/heikkilae.html -- 14.3 Кб -- 08.12.2003
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    15. http://www.mrao.cam.ac.uk/yerac/heikkilae/heikkilae.ps
    ... The proximity of the LMC enables detailed studies of the molecular gas in an environment differing from that in quiescent spiral galaxies such as the Milky Way. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/yerac/heikkilae/heikkilae.ps -- 286.8 Кб -- 22.02.1995
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    16. Small scale distribution in Molecular Clouds
    ... Another interesting case is edge-on spiral galaxies which are so distant (angular size of about one arcminute) that their ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/thoraval/thoraval.html -- 20.5 Кб -- 08.12.2003
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    17. http://www.mrao.cam.ac.uk/yerac/thoraval/thoraval.ps
    ... Another interesting case is edge­on spiral galaxies which are so distant (angular size of about one arcminute) that their ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/yerac/thoraval/thoraval.ps -- 1130.5 Кб -- 22.02.1995
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    18. Neutral hydrogen absorption in the Seyfert nucleus of NGC 4151
    ... Seyfert galaxies, discovered optically by Carl Seyfert in 1943 ( Seyfert (1943) ) in spiral galaxies exhibiting bright nuclei with broad emission lines in their spectra, are not as powerful as radio galaxies or quasars (in fact they are radio quiet - but ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/mundell/mundell.html -- 22.6 Кб -- 08.12.2003
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    19. http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2005/MidIRSocorroNov05.pdf
    ... 12 14 16 NGC 2798 10 5 -1 NGC 3351 ) S (MJy sr Spitzer Near Galaxies Legacy Survey: nu2 clear IRS spectra of (a random subsample 1 of) spiral galaxies. 4 6 8 10 (µm) 12 14 16 0.5 NGC 7793 Socorro 2005: Mid-IR Emission from Galaxies ­ p. 24 Sample Mid-IR ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2005/MidIRSocorroNov05.pdf -- 1996.8 Кб -- 25.11.2009
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    20. http://www.mrao.cam.ac.uk/yerac/mundell/mundell.ps
    ... Seyfert galaxies, discovered optically by Carl Seyfert in 1943 (Seyfert (1943)) in spiral galaxies exhibiting bright nuclei with broad emission lines in their spectra, are not as powerful as radio galaxies or quasars (in fact they are radio quiet --- but ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/yerac/mundell/mundell.ps -- 397.3 Кб -- 22.02.1995
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