... Brief review on merger rate of galaxiesMergers of luminous early-type galaxies in ... to construct a large and volume-limited complete massive early-type galaxymergers ...
[
Текст
]
Ссылки http://www.atnf.csiro.au/research/Astro2008/Postings/Zhonglue_Wen.pdf -- 1332.8 Кб -- 26.06.2008 Похожие документы
... Julie Comerford (UC Berkeley): "A New Way of Identifying GalaxyMergers: Offset AGN in GalaxyMerger Remnants in the DEEP2 ... Raffaella Morganti (ASTRON): "Galaxymergers and radio galaxies" . Lakshmi Saripalli (RRI): "X-shaped radio sources" . 4. ...
... A New Way of Identifying GalaxyMergers: Offset AGN in GalaxyMerger Remnants in the DEEP2 Galaxy Redshift Survey . ... Title . 09:00 (30min) . Raffaella Morganti . GalaxyMergers and Radio Galaxies . 09:30 (30min) . Daniel Yardley . ...
... Although galaxymergers are thought to play an important role in forming elliptical galaxies, mergers in galaxy clusters have drawn less attention compared to mergers in field environments due to high peculiar velocities of cluster galaxies. ...
... in ULIRGs formed by gas-rich galaxymergers and thereby discuss what powers ULIRGs ... For example, more massive galaxymergers are more likely to become AGN-dominated ...
... Table 4 lists a few strongly interacting or merginggalaxies which also show broad H I absorption lines. ... the starburst is driven inwards by strong tidal interaction or merging between galaxies (see e.g., Rieke et al. 1985), whereas ...
... Galaxymerger rates How many binary BHs from galaxymergers? ... Black-hole mass function (BH mass, z) + Galaxymerger rate f (galaxy mass, z) => Predicted black-hole merger rate (z, BH mass ...
[
Текст
]
Ссылки http://www.atnf.csiro.au/research/Astro2008/Postings/Scott_Croom_Disc.pdf -- 181.9 Кб -- 26.06.2008 Похожие документы
... ATCA unravels the role of cold gas in a merging hyper-luminous radio galaxy at z=2 ... that a gas-rich (`wet') merger of galaxies is driving the rapid evolution of the ...
... Major mergers on massive early-type galaxies in clusters. ... galaxies in massive clusters at z=0.1 showing morphological signs of major mergers ... conclusion is that we can reproduce the fraction of galaxies with merger features ...