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    91. ATNF Colloquium
    ... If nearly all galaxies host a supermassive black . hole (SMBH) in their center, it is expected that pairs of SMBHs will be . ... hole (SMBH) in their center, it is expected that pairs of SMBHs will be . formed in the course of a merger event. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/news.php?action=show_item&item_id=750 -- 27.3 Кб -- 12.04.2016
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    92. http://www.atnf.csiro.au/research/Astro2008/Postings/Hiroshi_Sudou.pdf
    ... micro-arcsec (0.05 pc @ 100 Mpc) 3C66B, the First Challenge Target : 3C66B · z~0.02, radio galaxy (giant E) Calibrator : 3C66A · z~0.3, FSRQ Very close pair · Separation is only 0.1 degree · Accuracy of <10 micro-as achievable, in princple 6 epochs during ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/Astro2008/Postings/Hiroshi_Sudou.pdf -- 2456.2 Кб -- 26.06.2008
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    93. http://www.atnf.csiro.au/people/Enno.Middelberg/pubs/norris2006b/norris2006b.pdf
    ... Thus, we count a classical triple radio-loud source as being a radio source consisting of three radio components, but count a pair of interacting starburst galaxies as being two sources, each with one radio component. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Enno.Middelberg/pubs/norris2006b/norris2006b.pdf -- 585.2 Кб -- 24.11.2006
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    94. Some research projects
    ... Structure and Dynamics of Galaxies . HI studies of other individual galaxies . ... HI studies of other individual galaxies . NGC 253 -- NGC 922 -- NGC 986A . ... HI studies of interacting galaxies . NGC 1189 Group (HCG22) . ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Baerbel.Koribalski/research-old.html -- 4.9 Кб -- 27.02.2014
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    95. Pulsar Group Main/Animations
    ... Two galaxies, each containing a black hole at their centre, merge. ... another at the centre of the merged galaxy, sending out gravitational waves as they ... These gravitational waves eventually reach our Galaxy, the Milky Way, where they ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/pulsar/index.html?n=Main.Animations -- 12.9 Кб -- 01.03.2014
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    96. http://www.atnf.csiro.au/people/Peter.Kamphuis/Thesis/ch6.pdf
    ... 2002). In merging galaxies gas can be found almost anywhere around the merging pair and in the most fantastic distributions. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Peter.Kamphuis/Thesis/ch6.pdf -- 435.5 Кб -- 21.10.2013
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    97. Radio-excess infrared galaxies: a new population of active galaxies?
    ... Of the 12 objects in our main sample, we found that two are S0, two are elliptical galaxies, one is a strongly interacting pair, and one appears stellar and is classified spectroscopically as a BL Lac object. ...
    [ 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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    98. HI in shell galaxies
    ... Other optically interesting elliptical galaxies with detected HI are IC 1459, which appears to be an S0 but shows low contrast spiral arms and a counter-rotating core (illustrated in Malin 1985) and the interacting pair NGC 1549-1553 (in Malin & Carter ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/14_1/malin/paper/node2.html -- 56.1 Кб -- 08.04.2016
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    99. ATNF Science Highlights 2002
    ... Figure 2 The two-point correlation function for HIPASS galaxies, plotted as a function of transverse (оѓ) and radial (оЂ) pair separation. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/highlights/2002/zwaan/zwaan.html -- 53.0 Кб -- 08.04.2016
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    100. http://www.atnf.csiro.au/pasa/16_1/rivers/paper.pdf
    ... Five On­Off pairs created from the sequence ensure that a real galaxy will appear twice, once as a positive signal, and again as a negative one, referenced against two independent scans. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/pasa/16_1/rivers/paper.pdf -- 197.7 Кб -- 25.05.1999
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