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Post-starburst galaxies in different environments

Proceedings of the International Astronomical Union, 2019
AbstractPost-starburst galaxies (PSBGs) are systems that experienced a burst followed by a rapid quenching of star formation. However, it is still unclear what causes these events and what is the environmental role in the origin of PSBGs. To address this, we analysed sizes, morphologies, ages, and metallicities of PSBGs at 0.05 ≤ z ≤ 0.1 in groups and ...
Rodolfo Spindler   +2 more
openaire   +1 more source

Red Post-Starburst Galaxies

Astrophysics and Space Science, 1994
Observations of nearby star-forming regions suggest that the initial mass function is deficient in low-mass stars when the ambient star formation rate is high. We investigate the consequences of a truncated initial mass function on the photometric evolution of star burst galaxies using new models of stellar population synthesis. A major prediction with
openaire   +1 more source

The UV enigma of post-starburst galaxies

Astrophysics and Space Science, 2014
We have studied the panchromatic broad-band properties from the FUV to the MIR of a sample of 808 post-starburst galaxies. We find that in the optical and near-IR bands post-starburst galaxies (PSGs) form a remarkably uniform class of objects and that, on average, simple populations synthesis models (SSP) reproduce very well the SEDs of PSGs over a ...
Melnick, J, De Propris, R
openaire   +1 more source

Post-starburst galaxies and the galaxy color bimodality

Il Nuovo Cimento B, 2008
We present results from a multi-wavelength observing campaign of a sample of post-starburst galaxies. The origin and redshift evolution of the bimodal galaxy color distribution is at the focus of current extragalactic and cosmological research. Post-starburst galaxies have just experienced a strong and abruptly truncated starburst, causing them to ...
openaire   +1 more source

Post-Starburst Galaxies: Why Aren’t They Forming Stars?

AIP Conference Proceedings, 2010
We present high spatial resolution 21 cm HI observations of EA01A and EA01B, a pair of interacting post‐starburst, PSG or E+A, galaxies at z = 0.0746. Based on optical HST/WFPC2 images, both galaxies are known to display disturbed morphologies. They also appear to be linked by a bridge of stars.
S. De Rijcke   +6 more
openaire   +1 more source

A population of red candidate massive galaxies ~600 Myr after the Big Bang

Nature, 2023
Ivo Labbe   +2 more
exaly  

Simulations of the formation, evolution and clustering of galaxies and quasars

Nature, 2005
Volker Springel   +2 more
exaly  

Properties of galaxies reproduced by a hydrodynamic simulation

Nature, 2014
Mark Vogelsberger   +2 more
exaly  

High molecular gas fractions in normal massive star-forming galaxies in the young Universe

Nature, 2010
Linda Tacconi   +2 more
exaly  

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