scholarly journals STELLAR POPULATIONS ACROSS THE BLACK HOLE MASS–VELOCITY DISPERSION RELATION

2016 ◽  
Vol 832 (1) ◽  
pp. L11 ◽  
Author(s):  
Ignacio Martín-Navarro ◽  
Jean P. Brodie ◽  
Remco C. E. van den Bosch ◽  
Aaron J. Romanowsky ◽  
Duncan A. Forbes
2015 ◽  
Vol 11 (S319) ◽  
pp. 60-60
Author(s):  
Chiaki Kobayashi ◽  
Philip Taylor

AbstractIn our cosmological, chemodynamical simulations, (i) the black hole mass–velocity dispersion relation does not evolve, and black holes actually grow along the relation. (ii) the stellar mass–metallicity relation does not change its shape, while the gas-phase relation has a steeper slope at higher redshifts. (iii) While stellar metallicity gradients are made shallower by galaxy mergers, gas-phase gradients are affected more strongly by AGN feedback.


2015 ◽  
Vol 801 (1) ◽  
pp. 38 ◽  
Author(s):  
Jong-Hak Woo ◽  
Yosep Yoon ◽  
Songyoun Park ◽  
Daeseong Park ◽  
Sang Chul Kim

2004 ◽  
Vol 615 (2) ◽  
pp. 645-651 ◽  
Author(s):  
Christopher A. Onken ◽  
Laura Ferrarese ◽  
David Merritt ◽  
Bradley M. Peterson ◽  
Richard W. Pogge ◽  
...  

2002 ◽  
Vol 574 (2) ◽  
pp. 740-753 ◽  
Author(s):  
Scott Tremaine ◽  
Karl Gebhardt ◽  
Ralf Bender ◽  
Gary Bower ◽  
Alan Dressler ◽  
...  

2012 ◽  
Vol 201 (2) ◽  
pp. 29 ◽  
Author(s):  
Chelsea E. Harris ◽  
Vardha N. Bennert ◽  
Matthew W. Auger ◽  
Tommaso Treu ◽  
Jong-Hak Woo ◽  
...  

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