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    11. The Relation between the Large-scale Gas Dynamics, Nuclear Kinematics, and
    ... I compare the group of nearby starburst galaxies with distant ultra-luminous galaxies (Arp 220, NGC 6240, etc.), in which strong tidal interactions cause the radial gas inflow. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Baerbel.Koribalski/min_lecture/ -- 6.4 Кб -- 03.02.2013
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    12. http://www.atnf.csiro.au/people/Ray.Norris/papers/n239.pdf
    ... Even Arp 220 has a S20 cm /S3.6µm ratio a factor of 20 below the most moderate IFRS, and a factor of 4000 below the most ... Even in Arp 220, where as much as 100 magnitudes of extinction obscure the nucleus (e.g. Haas et al. 2001), the outer shell of ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Ray.Norris/papers/n239.pdf -- 1557.6 Кб -- 03.05.2011
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    13. http://www.atnf.csiro.au/people/Baerbel.Koribalski/min_lecture/min_lecture_final.ps.gz
    ... galaxies with distant ultra­luminous galaxies (Arp 220, NGC 6240, etc.), in which ... 300 10 NGC 3690/IC 694 42 .IB.9P. 300 1,5,8 IC 4553 (=Arp 220) 72 .S?.. ... in the distant ultra­luminous galaxies like Arp 220, NGC 6240, and others (see Table ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Baerbel.Koribalski/min_lecture/min_lecture_final.ps.gz -- 686.0 Кб -- 17.11.2001
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    14. A Global Model
    ... Whereas in the distant ultra-luminous galaxies like Arp 220, NGC 6240, and others (see Table 4) strong tidal interactions or merging are responsible for the central activity, the less violent starbursts in nearby galaxies like NGC 253 and NGC 1808 (see ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Baerbel.Koribalski/min_lecture/node27.html -- 10.8 Кб -- 04.02.2013
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    15. http://www.atnf.csiro.au/research/publications/ATNF_Publications_2011.pdf
    ... P) 217 Ott, J.; Henkel, C.; Braatz, J.A.; Weiъ, A. "Ammonia as a temperature tracer in the ultraluminous galaxy merger Arp 220". ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/publications/ATNF_Publications_2011.pdf -- 110.7 Кб -- 05.09.2012
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    16. http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/divulgacion/GALAXIAS_DEL_UNIVERSO_LOCAL_pp_26-35_Astronomia_102_DIC_07_bajaresolucion.pdf
    ... Estos objetos muestran una formaciСn estelar muy elevada y claros indicios de interacciones, como Las Antenas (Figura 7) o Arp 220. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/divulgacion/GALAXIAS_DEL_UNIVERSO_LOCAL_pp_26-35_Astronomia_102_DIC_07_bajaresolucion.pdf -- 1352.9 Кб -- 21.11.2007
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    17. http://www.atnf.csiro.au/projects/askap/archive/skanal.pdf
    ... Science working document suggests that a stand-alone SKA should detect: Moderate-luminosity OH megamasers (like Arp 220) will be detected at 20 Jy at z=2 at 10 km s;1 : This assumes a frequency range of 530 MHz to 1.6 GHz. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/projects/askap/archive/skanal.pdf -- 328.8 Кб -- 19.03.2002
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    18. http://www.atnf.csiro.au/projects/askap/archive/skanal.ps
    ... Science working document suggests that a stand­alone SKA should detect: ffl Moderate­luminosity OH megamasers (like Arp 220) will be detected at 20ЇJy at z=2 at 10 km s \Gamma1 : This assumes a frequency range of 530 MHz to 1.6 GHz. ffl Moderate ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/projects/askap/archive/skanal.ps -- 1072.1 Кб -- 19.03.2002
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    19. Radio-excess infrared galaxies: a new population of active galaxies?
    ... On the basis of radio and optical imaging and spectroscopy and from the FIR colours, they propose that these objects may form an evolutionary link between ultraluminous infrared galaxies, like Arp 220, and quasars. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Ray.Norris/papers/n118/n118.html -- 104.9 Кб -- 28.02.2014
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    20. http://www.atnf.csiro.au/people/Ray.Norris/papers/n260.pdf
    ... sensitivities increase, VLBI observations have become more sensitive to detection of radio supernovae in the relatively nearby Universe, such as those in Arp 220 (Smith et al. 1998b), and so a VLBI detection no longer unambiguously implies an AGN ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Ray.Norris/papers/n260.pdf -- 2610.6 Кб -- 22.03.2011
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