Results 41 to 50 of about 1,551 (227)
The environmental dependence of rapidly quenching and rejuvenating galaxies [PDF]
ABSTRACT By combining H α flux measurements from the Sloan Digital Sky Survey (SDSS) with ultraviolet (UV) flux observations from the Galaxy Evolution Explorer (GALEX), we examine the environmental dependence (through central/satellite distinction) of the rapid quenching and rejuvenation of galaxies.
Cleland, Cressida, McGee, Sean
openaire +2 more sources
Quenching time-scales of galaxies in the eagle simulations
Final version accepted to MNRAS.
Ruby J Wright +5 more
openaire +4 more sources
There was a star-forming galaxy that was quenched
Cluster galaxies are subject to a whole range of processes and interactions that dramatically change their properties. To shed light on these issues, we analyze the most homogeneous and complete local cluster galaxy survey to date: WINGS/OmegaWINGS, and use stellar population synthesis techniques to obtain properties such as stellar mass, stellar ages,
Pérez-Millán, David +2 more
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The Roles of Mass and Environment in the Quenching of Galaxies. II. [PDF]
Abstract We take advantage of an analytic model of galaxy formation coupled to the merger tree of an N-body simulation to study the roles of environment and stellar mass in the quenching of galaxies. The model has been originally set in order to provide the observed evolution of the stellar mass function as well as reasonable predictions
E. Contini +5 more
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The enhancement of rapidly quenched galaxies in distant clusters at 0.5 < z < 1.0 [PDF]
Funding: MS acknowledges support from IAC and STFC. VW acknowledges support from the European Research Council Starting grant (SEDmorph, P.I. V. Wild).We investigate the relationship between environment and galaxy evolution in the redshift range 0.5 < z <
William G Hartley +13 more
core +1 more source
The imprint of cosmic web quenching on central galaxies
ABSTRACT We investigate how cosmic web environment impacts the average properties of central galaxies in the Sloan Digital Sky Survey (SDSS). We analyse how the average specific star formation rate, stellar age, metallicity, and element abundance ratio [α/Fe] of SDSS central galaxies depend on distance from the cosmic web nodes, walls ...
N Winkel +5 more
openaire +4 more sources
This review explores advances in wearable and lab‐on‐chip technologies for breast cancer detection. Covering tactile, thermal, ultrasound, microwave, electrical impedance tomography, electrochemical, microelectromechanical, and optical systems, it highlights innovations in flexible electronics, nanomaterials, and machine learning.
Neshika Wijewardhane +4 more
wiley +1 more source
A STELLAR MASS THRESHOLD FOR QUENCHING OF FIELD GALAXIES [PDF]
We demonstrate that dwarf galaxies (10^7 < M_stellar < 10^9 Msun) with no active star formation are extremely rare (<0.06%) in the field. Our sample is based on the NASA-Sloan Atlas which is a re-analysis of the Sloan Digital Sky Survey Data Release 8.
Geha, M. +3 more
openaire +2 more sources
The impact of quenching on galaxy profiles in the
ABSTRACT We study specific star formation rate (sSFR) and gas profiles of star-forming (SF) and green valley (GV) galaxies in the simba cosmological hydrodynamic simulation. SF galaxy half-light radii (Rhalf) at z = 0 and their evolution (∝(1 + z)−0.78) agree with observations.
Sarah Appleby +4 more
openaire +4 more sources
Multiple mechanisms quench passive spiral galaxies [PDF]
15 pages, 7 figures, accepted for publication in ...
Fraser-McKelvie, Amelia +4 more
openaire +5 more sources

