scholarly journals ROLE OF GALAXY MERGERS IN COSMIC STAR FORMATION HISTORY

2009 ◽  
Vol 697 (2) ◽  
pp. 1764-1783 ◽  
Author(s):  
Yong Shi ◽  
George Rieke ◽  
Jennifer Lotz ◽  
Pablo G. Perez-Gonzalez
2014 ◽  
Vol 789 (2) ◽  
pp. 96 ◽  
Author(s):  
Hakim Atek ◽  
Jean-Paul Kneib ◽  
Camilla Pacifici ◽  
Matthew Malkan ◽  
Stephane Charlot ◽  
...  

1999 ◽  
Vol 186 ◽  
pp. 202-202
Author(s):  
Yasuhiro Shioya ◽  
Kenji Bekki

We investigate the nature of stellar populations of major galaxy mergers between late-type spirals considerably abundant in interstellar medium by performing numerical simulations designed to solve both the dynamical and chemical evolution in a self-consistent manner. We particularly consider that the star formation history of galaxy mergers is a crucial determinant for the nature of stellar populations of merger remnants, and therefore investigate how the difference in star formation history between galaxy mergers affects the chemical evolution of galaxy mergers.


2013 ◽  
Vol 14 (1) ◽  
pp. 15-34 ◽  
Author(s):  
Lu-Lu Fan ◽  
Andrea Lapi ◽  
Alessandro Bressan ◽  
Mario Nonino ◽  
Gianfranco De Zotti ◽  
...  

2015 ◽  
Vol 579 ◽  
pp. A132 ◽  
Author(s):  
P. Popesso ◽  
A. Biviano ◽  
A. Finoguenov ◽  
D. Wilman ◽  
M. Salvato ◽  
...  

2019 ◽  
Vol 15 (S356) ◽  
pp. 224-224
Author(s):  
Allison Man

AbstractRadio galaxies are ideal sites to scrutinize AGN feedback physics, as they are massive galaxies with jets that interact with the surrounding ISM. I will present a detailed analysis of the recent star formation history and conditions of a starbursting, massive radio galaxy at z = 2.6, PKS 0529-549. In the 8.5-hour VLT/X-Shooter spectrum, we detect unambiguous signatures of stellar photospheric absorption lines originating from OB-stars. Comparison with model spectra shows that more than one burst took place in its recent past: the most recent one at 4 − 7 Myr, and another aged ⩾20 Myr. ALMA observations of the [CI] atomic carbon emission line indicates that it has a low molecular gas fraction (∼13%) and short depletion time (∼40 Myr). Most intriguing is the modest velocity dispersion (⩽50 km/s) of these photospheric lines and the ALMA [CI] cold gas. We attribute its efficient star formation to compressive gas motions, induced by radio jets and/or interaction. Star formation works in concert with the AGN to remove any residual molecular gas and eventually leads to quenching.


2021 ◽  
Vol 909 (2) ◽  
pp. 192 ◽  
Author(s):  
C. Gallart ◽  
M. Monelli ◽  
T. Ruiz-Lara ◽  
A. Calamida ◽  
S. Cassisi ◽  
...  

2009 ◽  
Vol 394 (4) ◽  
pp. 1713-1720 ◽  
Author(s):  
Sugata Kaviraj ◽  
Sebastien Peirani ◽  
Sadegh Khochfar ◽  
Joseph Silk ◽  
Scott Kay

2015 ◽  
Vol 450 (3) ◽  
pp. 2749-2763 ◽  
Author(s):  
V. Guglielmo ◽  
B. M. Poggianti ◽  
A. Moretti ◽  
J. Fritz ◽  
R. Calvi ◽  
...  

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