Dynamics and morphology of galactic mergers

1995 ◽  
Vol 108 (10) ◽  
pp. 1207-1223
Author(s):  
A. Curir ◽  
F. de Felice ◽  
A. Ferrari ◽  
S. Fogliani
Keyword(s):  
Galactic Mergers

scholarly journals The Survival of the Core Fundamental Plane against Galactic Mergers

1999 ◽  
Vol 517 (1) ◽  
pp. 92-102 ◽  
Author(s):  
Kelly Holley‐Bockelmann ◽  
Douglas Richstone
Keyword(s):  
Fundamental Plane ◽  
The Core ◽  
Galactic Mergers

The M / L * Ratio of Young Star Clusters in Galactic Mergers

2005 ◽  
Vol 620 (1) ◽  
pp. L27-L30 ◽  
Author(s):  
C. M. Boily ◽  
A. Lançon ◽  
S. Deiters ◽  
D. C. Heggie
Keyword(s):  
Star Clusters ◽  
Young Star ◽  
Young Star Clusters ◽  
Galactic Mergers

Galactic Mergers at redshift z ∼ 5, a sample of fast growing QSOs

2019 ◽  
Vol 15 (S356) ◽  
pp. 291-291
Author(s):  
Nathen Nguyen
Keyword(s):  
Black Holes ◽  
Star Formation ◽  
Emission Line ◽  
Galaxy Evolution ◽  
Far Infrared ◽  
Supermassive Black Holes ◽  
Fast Growing ◽  
Multi Wavelength ◽  
Cold Gas ◽  
Galactic Mergers

AbstractIn order to construct accurate Galaxy Evolution models, a more thorough understanding of the high SFRs seen at z > 2 is needed. To better understand AGNs at higher redshifts, we have conducted a multi-wavelength of 38 of the most luminous AGNs found in the SDSS catalogue at redshift z ∼ 4.8, powered by fast-growing supermassive black holes (SMBHs). Using Herschel/SPIRE observations, we found star formation rates (SFRs) of up to 4000 Solar masses per year. We believe that both the AGN and star formation of these objects are fed by a common reservoir of cold gas, and that this cold gas is due to in-falling matter from major mergers. In this talk, we present ALMA band-7 data of the [CII] λ157.74 m emission line and underlying far-infrared (FIR) continuum of twelve luminous quasars at z∼4.8 in our search for dynamically interacting companions.

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