Results 41 to 50 of about 14,525 (205)
The Mass Dependance of Satellite Quenching in Milky Way-like Halos [PDF]
, 2014 Using the Sloan Digital Sky Survey, we examine the quenching of satellite galaxies around isolated Milky Way-like hosts in the local Universe. We find that the efficiency of satellite quenching around isolated galaxies is low and roughly constant over ...
Boylan-Kolchin, Michael +5 more
core +1 more source
Gone after one orbit: How cluster environments quench galaxies [PDF]
, 2019 The effect of galactic orbits on a galaxy's internal evolution within a galaxy cluster environment has been the focus of heated debate in recent years.
Biviano, Andrea +4 more
core +2 more sources
Bursting and quenching in satellite galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2019 ABSTRACT The difference in stellar metallicity between red and blue galaxies with the same mass constrains the time-scale over which red galaxies ceased to form stars. Here we investigate this constraint with the galics 2.0 semi-analytic model of galaxy formation.
Koutsouridou, I, Cattaneo, A
openaire +3 more sources
AGN quenching in simulated dwarf galaxies
, 2022 23 pages, 11 figures; submitted to ...
Sharma, Ray S. +4 more
openaire +2 more sources
, 2017 Recent studies suggest that the quenching properties of galaxies are correlated over several mega-parsecs. The large-scale "galactic conformity" phenomenon around central galaxies has been regarded as a potential signature of "galaxy assembly bias" or ...
Mandelbaum, Rachel, Zu, Ying
core +1 more source
The Hubble Sequence in Groups: The Birth of the Early-Type Galaxies [PDF]
, 2010 The physical mechanisms and timescales that determine the morphological signatures and the quenching of star formation of typical (~L*) elliptical galaxies are not well understood.
Carollo, C. M., Feldmann, R., Mayer, L.
core +2 more sources
, 2014 Recent observations suggested that star formation quenching in galaxies is related to galaxy structure. Here we propose a new mechanism to explain the physical origin of this correlation. We assume that while quiescent galaxies are maintained quenched by
Guo, Fulai
core +1 more source
Do cluster properties affect the quenching rate? [PDF]
, 2014 The quenching rate is known to depend on galaxy stellar mass and environment, however, possible dependences on the hosting halo properties, such as mass, richness, and dynamical status, are still debated.
Andreon, S., Raichoor, A.
core +3 more sources
The LEGA-C galaxy survey: Multiple quenching channels for quiescent galaxies at z ∼ 1
Astronomy & AstrophysicsAims. We analyzed the sizes and star formation histories (SFHs) of 2908 galaxies with M★ ≥ 109 M⊙ at 0.6
Nersesian Angelos +11 more
doaj +1 more source
Mapping stellar content to dark matter halos. II. Halo mass is the main driver of galaxy quenching
, 2015 We develop a simple yet comprehensive method to distinguish the underlying drivers of galaxy quenching, using the clustering and galaxy-galaxy lensing of red and blue galaxies in SDSS.
Mandelbaum, Rachel, Zu, Ying
core +2 more sources