THE GRISM LENS-AMPLIFIED SURVEY FROM SPACE (GLASS). V. EXTENT AND SPATIAL DISTRIBUTION OF STAR FORMATION IN z ∼ 0.5 CLUSTER GALAXIES

ABSTRACT We present the first study of the spatial distribution of star formation in z ∼ 0.5 cluster galaxies. The analysis is based on data taken with the Wide Field Camera 3 as part of the Grism Lens-Amplified Survey from Space (GLASS). We illustrate the methodology by focusing on two clusters (MA...

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Published inThe Astrophysical journal Vol. 814; no. 2; pp. 161 - 19
Main Authors Vulcani, Benedetta, Treu, Tommaso, Schmidt, Kasper B., Poggianti, Bianca M., Dressler, Alan, Fontana, Adriano, Bradač, Marusa, Brammer, Gabriel B., Hoag, Austin, Huang, Kuan-Han, Malkan, Matthew, Pentericci, Laura, Trenti, Michele, Linden, Anja von der, Abramson, Louis, He, Julie, Morris, Glenn
Format Journal Article
LanguageEnglish
Published United States The American Astronomical Society 01.12.2015
Institute of Physics (IOP)
Subjects
ASTRONOMY AND ASTROPHYSICS
Continuums
Emission
Galactic clusters
Galaxies
galaxies: clusters: general
galaxies: evolution
galaxies: formation
galaxies: general
galaxies: star formation
Glass
Morphology
Star clusters
Star formation
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Abstract ABSTRACT We present the first study of the spatial distribution of star formation in z ∼ 0.5 cluster galaxies. The analysis is based on data taken with the Wide Field Camera 3 as part of the Grism Lens-Amplified Survey from Space (GLASS). We illustrate the methodology by focusing on two clusters (MACS 0717.5+3745 and MACS 1423.8+2404) with different morphologies (one relaxed and one merging) and use foreground and background galaxies as a field control sample. The cluster+field sample consists of 42 galaxies with stellar masses in the range 108-1011 M and star formation rates in the range 1-20 M yr−1. Both in clusters and in the field, H is more extended than the rest-frame UV continuum in 60% of the cases, consistent with diffuse star formation and inside-out growth. In ∼20% of the cases, the H emission appears more extended in cluster galaxies than in the field, pointing perhaps to ionized gas being stripped and/or star formation being enhanced at large radii. The peak of the H emission and that of the continuum are offset by less than 1 kpc. We investigate trends with the hot gas density as traced by the X-ray emission, and with the surface mass density as inferred from gravitational lens models, and find no conclusive results. The diversity of morphologies and sizes observed in H illustrates the complexity of the environmental processes that regulate star formation. Upcoming analysis of the full GLASS data set will increase our sample size by almost an order of magnitude, verifying and strengthening the inference from this initial data set.
AbstractList We present the first study of the spatial distribution of star formation in z ~ 0.5 cluster galaxies. The analysis is based on data taken with the Wide Field Camera 3 as part of the Grism Lens-Amplified Survey from Space (GLASS). We illustrate the methodology by focusing on two clusters (MACS 0717.5+3745 and MACS 1423.8+2404) with different morphologies (one relaxed and one merging) and use foreground and background galaxies as a field control sample. The cluster+field sample consists of 42 galaxies with stellar masses in the range 108–1011 M⊙ and star formation rates in the range 1–20 M⊙ yr–1. Both in clusters and in the field, Hα is more extended than the rest-frame UV continuum in 60% of the cases, consistent with diffuse star formation and inside-out growth. In ~20% of the cases, the Hα emission appears more extended in cluster galaxies than in the field, pointing perhaps to ionized gas being stripped and/or star formation being enhanced at large radii. Here, the peak of the Hα emission and that of the continuum are offset by less than 1 kpc. We investigate trends with the hot gas density as traced by the X-ray emission, and with the surface mass density as inferred from gravitational lens models, and find no conclusive results. The diversity of morphologies and sizes observed in Hα illustrates the complexity of the environmental processes that regulate star formation. Upcoming analysis of the full GLASS data set will increase our sample size by almost an order of magnitude, verifying and strengthening the inference from this initial data set.
We present the first study of the spatial distribution of star formation in z ~ 0.5 cluster galaxies. The analysis is based on data taken with the Wide Field Camera 3 as part of the Grism Lens-Amplified Survey from Space (GLASS). We illustrate the methodology by focusing on two clusters (MACS 0717.5+3745 and MACS 1423.8 +2404) with different morphologies (one relaxed and one merging) and use foreground and background galaxies as a field control sample. The cluster+field sample consists of 42 galaxies with stellar masses in the range 10 super(8)-10 super(11) M sub([middot in circle]) and star formation rates in the range 1-20 M sub([middot in circle]) yr super(-1). Both in clusters and in the field, H[alpha] is more extended than the rest-frame UV continuum in 60% of the cases, consistent with diffuse star formation and inside-out growth. In ~20% of the cases, the H[alpha] emission appears more extended in cluster galaxies than in the field, pointing perhaps to ionized gas being stripped and/or star formation being enhanced at large radii. The peak of the H[alpha] emission and that of the continuum are offset by less than 1 kpc. We investigate trends with the hot gas density as traced by the X-ray emission, and with the surface mass density as inferred from gravitational lens models, and find no conclusive results. The diversity of morphologies and sizes observed in H[alpha] illustrates the complexity of the environmental processes that regulate star formation. Upcoming analysis of the full GLASS data set will increase our sample size by almost an order of magnitude, verifying and strengthening the inference from this initial data set.
ABSTRACT We present the first study of the spatial distribution of star formation in z ∼ 0.5 cluster galaxies. The analysis is based on data taken with the Wide Field Camera 3 as part of the Grism Lens-Amplified Survey from Space (GLASS). We illustrate the methodology by focusing on two clusters (MACS 0717.5+3745 and MACS 1423.8+2404) with different morphologies (one relaxed and one merging) and use foreground and background galaxies as a field control sample. The cluster+field sample consists of 42 galaxies with stellar masses in the range 108-1011 M and star formation rates in the range 1-20 M yr−1. Both in clusters and in the field, H is more extended than the rest-frame UV continuum in 60% of the cases, consistent with diffuse star formation and inside-out growth. In ∼20% of the cases, the H emission appears more extended in cluster galaxies than in the field, pointing perhaps to ionized gas being stripped and/or star formation being enhanced at large radii. The peak of the H emission and that of the continuum are offset by less than 1 kpc. We investigate trends with the hot gas density as traced by the X-ray emission, and with the surface mass density as inferred from gravitational lens models, and find no conclusive results. The diversity of morphologies and sizes observed in H illustrates the complexity of the environmental processes that regulate star formation. Upcoming analysis of the full GLASS data set will increase our sample size by almost an order of magnitude, verifying and strengthening the inference from this initial data set.
Author He, Julie
Poggianti, Bianca M.
Vulcani, Benedetta
Dressler, Alan
Bradač, Marusa
Brammer, Gabriel B.
Schmidt, Kasper B.
Trenti, Michele
Hoag, Austin
Abramson, Louis
Linden, Anja von der
Pentericci, Laura
Treu, Tommaso
Huang, Kuan-Han
Fontana, Adriano
Morris, Glenn
Malkan, Matthew
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  givenname: Kuan-Han
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  organization: Department of Physics and Astronomy, University of California , Los Angeles, CA 90095-1547, USA
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  surname: Pentericci
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  organization: School of Physics, University of Melbourne , VIC 3010, Australia
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  organization: Kavli Institute for Particle Astrophysics and Cosmology, Stanford University , 452 Lomita Mall, Stanford, CA 94305-4085, USA
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  organization: Department of Physics, University of California , Davis, CA 95616, USA
– sequence: 17
  givenname: Glenn
  surname: Morris
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  organization: SLAC National Accelerator Laboratory , 2575 Sand Hill Road, Menlo Park, CA 94025, USA
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Snippet ABSTRACT We present the first study of the spatial distribution of star formation in z ∼ 0.5 cluster galaxies. The analysis is based on data taken with the...
We present the first study of the spatial distribution of star formation in z ~ 0.5 cluster galaxies. The analysis is based on data taken with the Wide Field...
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SubjectTerms ASTRONOMY AND ASTROPHYSICS
Continuums
Emission
Galactic clusters
Galaxies
galaxies: clusters: general
galaxies: evolution
galaxies: formation
galaxies: general
galaxies: star formation
Glass
Morphology
Star clusters
Star formation
Title THE GRISM LENS-AMPLIFIED SURVEY FROM SPACE (GLASS). V. EXTENT AND SPATIAL DISTRIBUTION OF STAR FORMATION IN z ∼ 0.5 CLUSTER GALAXIES
URI https://iopscience.iop.org/article/10.1088/0004-637X/814/2/161
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