Ultraviolet+infrared star formation rates: Hickson compact groups with swift and spitzer

P. Tzanavaris, A. E. Hornschemeier, S. C. Gallagher, K. E. Johnson, C. Gronwall, S. Immler, A. E. Reines, E. Hoversten, J. C. Charlton

Research output: Contribution to journalArticle

40 Citations (Scopus)

Abstract

We present Swift UVOT ultraviolet (UV; 1600-3000 Å) data with complete three-band UV photometry for a sample of 41 galaxies in 11 nearby (<4500 km s-1) Hickson Compact Groups (HCGs) of galaxies. We use UVOT uvw2-band (2000 Å) photometry to estimate the dust-unobscured component, SFRUV, of the total star formation rate, SFR TOTAL. We use Spitzer MIPS 24 μm photometry to estimate SFR IR, the component of SFRTOTAL that suffers dust extinction in the UV and is re-emitted in the IR. By combining the two components, we obtain SFRTOTAL estimates for all HCG galaxies. We obtain total stellar mass, M *, estimates by means of Two Micron All Sky Survey Ks -band luminosities, and use them to calculate specific star formation rates, SSFR ≡ SFRTOTAL/M *. SSFR values show a clear and significant bimodality, with a gap between low (≲3.2 × 10-11yr-1) and high-SSFR (≳1.2 × 10-10yr-1) systems. We compare this bimodality to the previously discovered bimodality in αIRAC, the MIR activity index from a power-law fit to the Spitzer IRAC 4.5-8 μm data for these galaxies. We find that all galaxies with αIRAC ≤ 0 ( >0) are in the high- (low-) SSFR locus, as expected if high levels of star-forming activity power MIR emission from polycyclic aromatic hydrocarbon molecules and a hot dust continuum. Consistent with this finding, all elliptical/S0 galaxies are in the low-SSFR locus, while 22 out of 24 spirals/irregulars are in the high-SSFR locus, with two borderline cases. We further divide our sample into three subsamples (I, II, and III) according to decreasing H I richness of the parent galaxy group to which a galaxy belongs. Consistent with the SSFR and αIRAC bimodality, 12 out of 15 type I (11 out of 12 type III) galaxies are in the high- (low-) SSFR locus, while type II galaxies span almost the full range of SSFR values. We use the Spitzer Infrared Nearby Galaxy Survey (SINGS) to construct a comparison subsample of galaxies that (1) match HCG galaxies in J-band total galaxy luminosity and (2) are not strongly interacting and largely isolated. This selection eliminates mostly low-luminosity dwarfs and galaxies with some degree of peculiarity, providing a substantially improved, quiescent control sample. Unlike HCG galaxies, galaxies in the comparison SINGS subsample are continuously distributed both in SSFR and αIRAC, although they show ranges in SFRTOTAL values, morphologies and stellar masses similar to those for HCG systems. We test the SSFR bimodality against a number of uncertainties, and find that these can only lead to its further enhancement. Excluding galaxies belonging to HCGs with three giant galaxies (triplets) leaves both the SSFR and the αIRAC bimodality completely unaffected. We interpret these results as further evidence that an environment characterized by high galaxy number densities and low galaxy velocity dispersions, such as the one found in compact groups, plays a key role in accelerating galaxy evolution by enhancing star formation processes in galaxies and favoring a fast transition to quiescence.

Original languageEnglish (US)
Pages (from-to)556-573
Number of pages18
JournalAstrophysical Journal
Volume716
Issue number1
DOIs
StatePublished - Jan 1 2010

Fingerprint

infrared stars
star formation rate
galaxies
PAH
dust
loci
luminosity
comparison
rate

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Tzanavaris, P. ; Hornschemeier, A. E. ; Gallagher, S. C. ; Johnson, K. E. ; Gronwall, C. ; Immler, S. ; Reines, A. E. ; Hoversten, E. ; Charlton, J. C. / Ultraviolet+infrared star formation rates : Hickson compact groups with swift and spitzer. In: Astrophysical Journal. 2010 ; Vol. 716, No. 1. pp. 556-573.
@article{298301358ecd4097bbf73db471273335,
title = "Ultraviolet+infrared star formation rates: Hickson compact groups with swift and spitzer",
abstract = "We present Swift UVOT ultraviolet (UV; 1600-3000 {\AA}) data with complete three-band UV photometry for a sample of 41 galaxies in 11 nearby (<4500 km s-1) Hickson Compact Groups (HCGs) of galaxies. We use UVOT uvw2-band (2000 {\AA}) photometry to estimate the dust-unobscured component, SFRUV, of the total star formation rate, SFR TOTAL. We use Spitzer MIPS 24 μm photometry to estimate SFR IR, the component of SFRTOTAL that suffers dust extinction in the UV and is re-emitted in the IR. By combining the two components, we obtain SFRTOTAL estimates for all HCG galaxies. We obtain total stellar mass, M *, estimates by means of Two Micron All Sky Survey Ks -band luminosities, and use them to calculate specific star formation rates, SSFR ≡ SFRTOTAL/M *. SSFR values show a clear and significant bimodality, with a gap between low (≲3.2 × 10-11yr-1) and high-SSFR (≳1.2 × 10-10yr-1) systems. We compare this bimodality to the previously discovered bimodality in αIRAC, the MIR activity index from a power-law fit to the Spitzer IRAC 4.5-8 μm data for these galaxies. We find that all galaxies with αIRAC ≤ 0 ( >0) are in the high- (low-) SSFR locus, as expected if high levels of star-forming activity power MIR emission from polycyclic aromatic hydrocarbon molecules and a hot dust continuum. Consistent with this finding, all elliptical/S0 galaxies are in the low-SSFR locus, while 22 out of 24 spirals/irregulars are in the high-SSFR locus, with two borderline cases. We further divide our sample into three subsamples (I, II, and III) according to decreasing H I richness of the parent galaxy group to which a galaxy belongs. Consistent with the SSFR and αIRAC bimodality, 12 out of 15 type I (11 out of 12 type III) galaxies are in the high- (low-) SSFR locus, while type II galaxies span almost the full range of SSFR values. We use the Spitzer Infrared Nearby Galaxy Survey (SINGS) to construct a comparison subsample of galaxies that (1) match HCG galaxies in J-band total galaxy luminosity and (2) are not strongly interacting and largely isolated. This selection eliminates mostly low-luminosity dwarfs and galaxies with some degree of peculiarity, providing a substantially improved, quiescent control sample. Unlike HCG galaxies, galaxies in the comparison SINGS subsample are continuously distributed both in SSFR and αIRAC, although they show ranges in SFRTOTAL values, morphologies and stellar masses similar to those for HCG systems. We test the SSFR bimodality against a number of uncertainties, and find that these can only lead to its further enhancement. Excluding galaxies belonging to HCGs with three giant galaxies (triplets) leaves both the SSFR and the αIRAC bimodality completely unaffected. We interpret these results as further evidence that an environment characterized by high galaxy number densities and low galaxy velocity dispersions, such as the one found in compact groups, plays a key role in accelerating galaxy evolution by enhancing star formation processes in galaxies and favoring a fast transition to quiescence.",
author = "P. Tzanavaris and Hornschemeier, {A. E.} and Gallagher, {S. C.} and Johnson, {K. E.} and C. Gronwall and S. Immler and Reines, {A. E.} and E. Hoversten and Charlton, {J. C.}",
year = "2010",
month = "1",
day = "1",
doi = "10.1088/0004-637X/716/1/556",
language = "English (US)",
volume = "716",
pages = "556--573",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "IOP Publishing Ltd.",
number = "1",

}

Tzanavaris, P, Hornschemeier, AE, Gallagher, SC, Johnson, KE, Gronwall, C, Immler, S, Reines, AE, Hoversten, E & Charlton, JC 2010, 'Ultraviolet+infrared star formation rates: Hickson compact groups with swift and spitzer', Astrophysical Journal, vol. 716, no. 1, pp. 556-573. https://doi.org/10.1088/0004-637X/716/1/556

Ultraviolet+infrared star formation rates : Hickson compact groups with swift and spitzer. / Tzanavaris, P.; Hornschemeier, A. E.; Gallagher, S. C.; Johnson, K. E.; Gronwall, C.; Immler, S.; Reines, A. E.; Hoversten, E.; Charlton, J. C.

In: Astrophysical Journal, Vol. 716, No. 1, 01.01.2010, p. 556-573.

Research output: Contribution to journalArticle

TY - JOUR

T1 - Ultraviolet+infrared star formation rates

T2 - Hickson compact groups with swift and spitzer

AU - Tzanavaris, P.

AU - Hornschemeier, A. E.

AU - Gallagher, S. C.

AU - Johnson, K. E.

AU - Gronwall, C.

AU - Immler, S.

AU - Reines, A. E.

AU - Hoversten, E.

AU - Charlton, J. C.

PY - 2010/1/1

Y1 - 2010/1/1

N2 - We present Swift UVOT ultraviolet (UV; 1600-3000 Å) data with complete three-band UV photometry for a sample of 41 galaxies in 11 nearby (<4500 km s-1) Hickson Compact Groups (HCGs) of galaxies. We use UVOT uvw2-band (2000 Å) photometry to estimate the dust-unobscured component, SFRUV, of the total star formation rate, SFR TOTAL. We use Spitzer MIPS 24 μm photometry to estimate SFR IR, the component of SFRTOTAL that suffers dust extinction in the UV and is re-emitted in the IR. By combining the two components, we obtain SFRTOTAL estimates for all HCG galaxies. We obtain total stellar mass, M *, estimates by means of Two Micron All Sky Survey Ks -band luminosities, and use them to calculate specific star formation rates, SSFR ≡ SFRTOTAL/M *. SSFR values show a clear and significant bimodality, with a gap between low (≲3.2 × 10-11yr-1) and high-SSFR (≳1.2 × 10-10yr-1) systems. We compare this bimodality to the previously discovered bimodality in αIRAC, the MIR activity index from a power-law fit to the Spitzer IRAC 4.5-8 μm data for these galaxies. We find that all galaxies with αIRAC ≤ 0 ( >0) are in the high- (low-) SSFR locus, as expected if high levels of star-forming activity power MIR emission from polycyclic aromatic hydrocarbon molecules and a hot dust continuum. Consistent with this finding, all elliptical/S0 galaxies are in the low-SSFR locus, while 22 out of 24 spirals/irregulars are in the high-SSFR locus, with two borderline cases. We further divide our sample into three subsamples (I, II, and III) according to decreasing H I richness of the parent galaxy group to which a galaxy belongs. Consistent with the SSFR and αIRAC bimodality, 12 out of 15 type I (11 out of 12 type III) galaxies are in the high- (low-) SSFR locus, while type II galaxies span almost the full range of SSFR values. We use the Spitzer Infrared Nearby Galaxy Survey (SINGS) to construct a comparison subsample of galaxies that (1) match HCG galaxies in J-band total galaxy luminosity and (2) are not strongly interacting and largely isolated. This selection eliminates mostly low-luminosity dwarfs and galaxies with some degree of peculiarity, providing a substantially improved, quiescent control sample. Unlike HCG galaxies, galaxies in the comparison SINGS subsample are continuously distributed both in SSFR and αIRAC, although they show ranges in SFRTOTAL values, morphologies and stellar masses similar to those for HCG systems. We test the SSFR bimodality against a number of uncertainties, and find that these can only lead to its further enhancement. Excluding galaxies belonging to HCGs with three giant galaxies (triplets) leaves both the SSFR and the αIRAC bimodality completely unaffected. We interpret these results as further evidence that an environment characterized by high galaxy number densities and low galaxy velocity dispersions, such as the one found in compact groups, plays a key role in accelerating galaxy evolution by enhancing star formation processes in galaxies and favoring a fast transition to quiescence.

AB - We present Swift UVOT ultraviolet (UV; 1600-3000 Å) data with complete three-band UV photometry for a sample of 41 galaxies in 11 nearby (<4500 km s-1) Hickson Compact Groups (HCGs) of galaxies. We use UVOT uvw2-band (2000 Å) photometry to estimate the dust-unobscured component, SFRUV, of the total star formation rate, SFR TOTAL. We use Spitzer MIPS 24 μm photometry to estimate SFR IR, the component of SFRTOTAL that suffers dust extinction in the UV and is re-emitted in the IR. By combining the two components, we obtain SFRTOTAL estimates for all HCG galaxies. We obtain total stellar mass, M *, estimates by means of Two Micron All Sky Survey Ks -band luminosities, and use them to calculate specific star formation rates, SSFR ≡ SFRTOTAL/M *. SSFR values show a clear and significant bimodality, with a gap between low (≲3.2 × 10-11yr-1) and high-SSFR (≳1.2 × 10-10yr-1) systems. We compare this bimodality to the previously discovered bimodality in αIRAC, the MIR activity index from a power-law fit to the Spitzer IRAC 4.5-8 μm data for these galaxies. We find that all galaxies with αIRAC ≤ 0 ( >0) are in the high- (low-) SSFR locus, as expected if high levels of star-forming activity power MIR emission from polycyclic aromatic hydrocarbon molecules and a hot dust continuum. Consistent with this finding, all elliptical/S0 galaxies are in the low-SSFR locus, while 22 out of 24 spirals/irregulars are in the high-SSFR locus, with two borderline cases. We further divide our sample into three subsamples (I, II, and III) according to decreasing H I richness of the parent galaxy group to which a galaxy belongs. Consistent with the SSFR and αIRAC bimodality, 12 out of 15 type I (11 out of 12 type III) galaxies are in the high- (low-) SSFR locus, while type II galaxies span almost the full range of SSFR values. We use the Spitzer Infrared Nearby Galaxy Survey (SINGS) to construct a comparison subsample of galaxies that (1) match HCG galaxies in J-band total galaxy luminosity and (2) are not strongly interacting and largely isolated. This selection eliminates mostly low-luminosity dwarfs and galaxies with some degree of peculiarity, providing a substantially improved, quiescent control sample. Unlike HCG galaxies, galaxies in the comparison SINGS subsample are continuously distributed both in SSFR and αIRAC, although they show ranges in SFRTOTAL values, morphologies and stellar masses similar to those for HCG systems. We test the SSFR bimodality against a number of uncertainties, and find that these can only lead to its further enhancement. Excluding galaxies belonging to HCGs with three giant galaxies (triplets) leaves both the SSFR and the αIRAC bimodality completely unaffected. We interpret these results as further evidence that an environment characterized by high galaxy number densities and low galaxy velocity dispersions, such as the one found in compact groups, plays a key role in accelerating galaxy evolution by enhancing star formation processes in galaxies and favoring a fast transition to quiescence.

UR - http://www.scopus.com/inward/record.url?scp=77952912281&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=77952912281&partnerID=8YFLogxK

U2 - 10.1088/0004-637X/716/1/556

DO - 10.1088/0004-637X/716/1/556

M3 - Article

AN - SCOPUS:77952912281

VL - 716

SP - 556

EP - 573

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 1

ER -