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Physical Explanation for the Galaxy Distribution on the and Diagrams or for the Limit on Orbital Anisotropy
Bitao Wang, Michele Cappellari, Yingjie Peng
In the and diagrams for characterizing dynamical states, the fast-rotator galaxies (both early-type and spirals) are distributed wit…
From haloes to galaxies -- II. The fundamental relations in star formation and quenching
Jing Dou, Yingjie Peng, Alvio Renzini +10
Star formation and quenching are two of the most important processes in galaxy formation and evolution. We explore in the local Universe the interrelationships among key integrated…
The 2175 Å dust feature in star-forming galaxies at : the dependence on stellar mass and specific star formation rate
Daichi Kashino, Simon J. Lilly, John D. Silverman +10
We present direct spectroscopic measurements of the broad 2175~Å absorption feature in 505 star-forming main-sequence galaxies at using individual and stacked spe…
The VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to
Sarah Leslie, Eva Schinnerer, Daizhong Liu +17
We provide a coherent, uniform measurement of the evolution of the logarithmic star formation rate (SFR) - stellar mass () relation, called the main sequence of star-forming g…
The weak imprint of environment on the stellar populations of galaxies
James Trussler, Roberto Maiolino, Claudia Maraston +4
We investigate the environmental dependence of the stellar populations of galaxies in SDSS DR7. Echoing earlier works, we find that satellites are both more metal-rich (<0.1 dex) a…
SDSS-IV MaNGA: The kinematic-morphology of galaxies on the mass vs star-formation relation in different environments
Bitao Wang, Michele Cappellari, Yingjie Peng +1
We study the link between the kinematic-morphology of galaxies, as inferred from integral-field stellar kinematics, and their relation between mass and star formation rate (SFR). O…