QUENCHING STAR FORMATION AT INTERMEDIATE REDSHIFTS: DOWNSIZING OF THE MASS FLUX DENSITY IN THE GREEN VALLEY

QUENCHING STAR FORMATION AT INTERMEDIATE REDSHIFTS: DOWNSIZING OF THE MASS FLUX DENSITY IN THE GREEN VALLEY

The bimodality in galaxy properties has been observed at low and high redshifts, with a clear distinction between star-forming galaxies in the blue cloud and passively evolving objects in the red sequence; the absence of galaxies with intermediate properties indicates that the quenching of star form...

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Published in:The Astrophysical journal Vol. 759; no. 1; pp. 1 - 12
Main Authors: GONCALVES, Thiago S, CHRISTOPHER MARTIN, D, MENENDEZ-DELMESTRE, Karín, WYDER, Ted K, KOEKEMOER, Anton
Format: Journal Article
Language:English
Published: Bristol IOP 01-11-2012
Subjects:
ASTRONOMY
ASTROPHYSICS
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
Clouds
COSMOLOGY
Downsizing
Earth, ocean, space
EMISSION SPECTROSCOPY
Exact sciences and technology
Flux
FLUX DENSITY
GALACTIC EVOLUTION
GALAXIES
LUMINOSITY
MASS
QUENCHING
RED SHIFT
Star formation
STARS
TELESCOPES
UNIVERSE
Valleys
Galaxy evolution
Spectroscopy
Red shift
Deimos
Galaxies
galaxies: luminosity function
galaxies: evolution
Mass transfer
Mars satellite
Flux density
Mass function
Star formation
Stellar mass
Age
Luminosity function
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Abstract The bimodality in galaxy properties has been observed at low and high redshifts, with a clear distinction between star-forming galaxies in the blue cloud and passively evolving objects in the red sequence; the absence of galaxies with intermediate properties indicates that the quenching of star formation and subsequent transition between populations must happen rapidly. In this paper, we present a study of over 100 transiting galaxies in the so-called green valley at intermediate redshifts (z ~ 0.8). By using very deep spectroscopy with the DEIMOS instrument at the Keck telescope we are able to infer the star formation histories of these objects and measure the stellar mass flux density transiting from the blue cloud to the red sequence when the universe was half its current age. Our results indicate that the process happened more rapidly and for more massive galaxies in the past, suggesting a top-down scenario in which the massive end of the red sequence is forming first. This represents another aspect of downsizing, with the mass flux density moving toward smaller galaxies in recent times.
AbstractList The bimodality in galaxy properties has been observed at low and high redshifts, with a clear distinction between star-forming galaxies in the blue cloud and passively evolving objects in the red sequence; the absence of galaxies with intermediate properties indicates that the quenching of star formation and subsequent transition between populations must happen rapidly. In this paper, we present a study of over 100 transiting galaxies in the so-called green valley at intermediate redshifts (z ~ 0.8). By using very deep spectroscopy with the DEIMOS instrument at the Keck telescope we are able to infer the star formation histories of these objects and measure the stellar mass flux density transiting from the blue cloud to the red sequence when the universe was half its current age. Our results indicate that the process happened more rapidly and for more massive galaxies in the past, suggesting a top-down scenario in which the massive end of the red sequence is forming first. This represents another aspect of downsizing, with the mass flux density moving toward smaller galaxies in recent times.
The bimodality in galaxy properties has been observed at low and high redshifts, with a clear distinction between star-forming galaxies in the blue cloud and passively evolving objects in the red sequence; the absence of galaxies with intermediate properties indicates that the quenching of star formation and subsequent transition between populations must happen rapidly. In this paper, we present a study of over 100 transiting galaxies in the so-called green valley at intermediate redshifts (z {approx} 0.8). By using very deep spectroscopy with the DEIMOS instrument at the Keck telescope we are able to infer the star formation histories of these objects and measure the stellar mass flux density transiting from the blue cloud to the red sequence when the universe was half its current age. Our results indicate that the process happened more rapidly and for more massive galaxies in the past, suggesting a top-down scenario in which the massive end of the red sequence is forming first. This represents another aspect of downsizing, with the mass flux density moving toward smaller galaxies in recent times.
Author KOEKEMOER, Anton
WYDER, Ted K
CHRISTOPHER MARTIN, D
MENENDEZ-DELMESTRE, Karín
GONCALVES, Thiago S
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  surname: MENENDEZ-DELMESTRE
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  givenname: Anton
  surname: KOEKEMOER
  fullname: KOEKEMOER, Anton
  organization: Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, United States
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Issue 1
Keywords Galaxy evolution
Spectroscopy
Red shift
Deimos
Galaxies
galaxies: luminosity function
galaxies: evolution
Mass transfer
Mars satellite
Flux density
Mass function
Star formation
Stellar mass
Age
Luminosity function
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Snippet The bimodality in galaxy properties has been observed at low and high redshifts, with a clear distinction between star-forming galaxies in the blue cloud and...
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SubjectTerms ASTRONOMY
ASTROPHYSICS
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
Clouds
COSMOLOGY
Downsizing
Earth, ocean, space
EMISSION SPECTROSCOPY
Exact sciences and technology
Flux
FLUX DENSITY
GALACTIC EVOLUTION
GALAXIES
LUMINOSITY
MASS
QUENCHING
RED SHIFT
Star formation
STARS
TELESCOPES
UNIVERSE
Valleys
Title QUENCHING STAR FORMATION AT INTERMEDIATE REDSHIFTS: DOWNSIZING OF THE MASS FLUX DENSITY IN THE GREEN VALLEY
URI https://search.proquest.com/docview/1709169446
https://search.proquest.com/docview/1718929591
https://www.osti.gov/biblio/22086446
Volume 759
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