Shocks and star formation in Stephan's quintet. I. Gemini spectroscopy of Hα-Bright knots

I. S. Konstantopoulos, P. N. Appleton, P. Guillard, G. Trancho, M. E. Cluver, N. Bastian, J. C. Charlton, K. Fedotov, S. C. Gallagher, L. J. Smith, C. J. Struck

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Abstract

We present a Gemini-GMOS spectroscopic study of Hubble Space Telescope (HST)-selected Hα-emitting regions in Stephan's Quintet (HCG 92), a nearby compact galaxy group, with the aim of disentangling the processes of shock-induced heating and star formation in its intra-group medium. The ≈40 sources are distributed across the system, but most densely concentrated in the ∼kiloparsec-long shock region. Their spectra neatly divide them into narrow- and broad-line emitters, and we decompose the latter into three or more emission peaks corresponding to spatial elements discernible in HST imaging. The emission-line ratios of the two populations of Hα-emitters confirm their nature as H II regions (90% of the sample) or molecular gas heated by a shock front propagating at ≲300 km s-1. Their redshift distribution reveals interesting three-dimensional structure with respect to gas-phase baryons, with no H II regions associated with shocked gas, no shocked regions in the intruder galaxy NGC 7318B, and a sharp boundary between shocks and star formation. We conclude that star formation is inhibited substantially, if not entirely, in the shock region. Attributing those H II regions projected against the shock to the intruder, we find a lopsided distribution of star formation in this galaxy, reminiscent of pileup regions in models of interacting galaxies. The Hα luminosities imply mass outputs, star formation rates, and efficiencies similar to nearby star-forming regions. Two large knots are an exception to this, being comparable in stellar output to the prolific 30 Doradus region. We also examine Stephan's Quintet in the context of compact galaxy group evolution, as a paradigm for intermittent star formation histories in the presence of a rich, X-ray-emitting intra-group medium. All spectra are provided as supplemental materials.

Original languageEnglish (US)
Article number1
JournalAstrophysical Journal
Volume784
Issue number1
DOIs
StatePublished - Mar 20 2014

Fingerprint

star formation
shock
spectroscopy
H II regions
compact galaxies
galactic clusters
Hubble Space Telescope
emitters
galaxies
interacting galaxies
output
shock fronts
molecular gases
star formation rate
baryons
luminosity
gas
histories
vapor phases
stars

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Konstantopoulos, I. S., Appleton, P. N., Guillard, P., Trancho, G., Cluver, M. E., Bastian, N., ... Struck, C. J. (2014). Shocks and star formation in Stephan's quintet. I. Gemini spectroscopy of Hα-Bright knots. Astrophysical Journal, 784(1), [1]. https://doi.org/10.1088/0004-637X/784/1/1
Konstantopoulos, I. S. ; Appleton, P. N. ; Guillard, P. ; Trancho, G. ; Cluver, M. E. ; Bastian, N. ; Charlton, J. C. ; Fedotov, K. ; Gallagher, S. C. ; Smith, L. J. ; Struck, C. J. / Shocks and star formation in Stephan's quintet. I. Gemini spectroscopy of Hα-Bright knots. In: Astrophysical Journal. 2014 ; Vol. 784, No. 1.
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abstract = "We present a Gemini-GMOS spectroscopic study of Hubble Space Telescope (HST)-selected Hα-emitting regions in Stephan's Quintet (HCG 92), a nearby compact galaxy group, with the aim of disentangling the processes of shock-induced heating and star formation in its intra-group medium. The ≈40 sources are distributed across the system, but most densely concentrated in the ∼kiloparsec-long shock region. Their spectra neatly divide them into narrow- and broad-line emitters, and we decompose the latter into three or more emission peaks corresponding to spatial elements discernible in HST imaging. The emission-line ratios of the two populations of Hα-emitters confirm their nature as H II regions (90{\%} of the sample) or molecular gas heated by a shock front propagating at ≲300 km s-1. Their redshift distribution reveals interesting three-dimensional structure with respect to gas-phase baryons, with no H II regions associated with shocked gas, no shocked regions in the intruder galaxy NGC 7318B, and a sharp boundary between shocks and star formation. We conclude that star formation is inhibited substantially, if not entirely, in the shock region. Attributing those H II regions projected against the shock to the intruder, we find a lopsided distribution of star formation in this galaxy, reminiscent of pileup regions in models of interacting galaxies. The Hα luminosities imply mass outputs, star formation rates, and efficiencies similar to nearby star-forming regions. Two large knots are an exception to this, being comparable in stellar output to the prolific 30 Doradus region. We also examine Stephan's Quintet in the context of compact galaxy group evolution, as a paradigm for intermittent star formation histories in the presence of a rich, X-ray-emitting intra-group medium. All spectra are provided as supplemental materials.",
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Konstantopoulos, IS, Appleton, PN, Guillard, P, Trancho, G, Cluver, ME, Bastian, N, Charlton, JC, Fedotov, K, Gallagher, SC, Smith, LJ & Struck, CJ 2014, 'Shocks and star formation in Stephan's quintet. I. Gemini spectroscopy of Hα-Bright knots', Astrophysical Journal, vol. 784, no. 1, 1. https://doi.org/10.1088/0004-637X/784/1/1

Shocks and star formation in Stephan's quintet. I. Gemini spectroscopy of Hα-Bright knots. / Konstantopoulos, I. S.; Appleton, P. N.; Guillard, P.; Trancho, G.; Cluver, M. E.; Bastian, N.; Charlton, J. C.; Fedotov, K.; Gallagher, S. C.; Smith, L. J.; Struck, C. J.

In: Astrophysical Journal, Vol. 784, No. 1, 1, 20.03.2014.

Research output: Contribution to journalArticle

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T1 - Shocks and star formation in Stephan's quintet. I. Gemini spectroscopy of Hα-Bright knots

AU - Konstantopoulos, I. S.

AU - Appleton, P. N.

AU - Guillard, P.

AU - Trancho, G.

AU - Cluver, M. E.

AU - Bastian, N.

AU - Charlton, J. C.

AU - Fedotov, K.

AU - Gallagher, S. C.

AU - Smith, L. J.

AU - Struck, C. J.

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N2 - We present a Gemini-GMOS spectroscopic study of Hubble Space Telescope (HST)-selected Hα-emitting regions in Stephan's Quintet (HCG 92), a nearby compact galaxy group, with the aim of disentangling the processes of shock-induced heating and star formation in its intra-group medium. The ≈40 sources are distributed across the system, but most densely concentrated in the ∼kiloparsec-long shock region. Their spectra neatly divide them into narrow- and broad-line emitters, and we decompose the latter into three or more emission peaks corresponding to spatial elements discernible in HST imaging. The emission-line ratios of the two populations of Hα-emitters confirm their nature as H II regions (90% of the sample) or molecular gas heated by a shock front propagating at ≲300 km s-1. Their redshift distribution reveals interesting three-dimensional structure with respect to gas-phase baryons, with no H II regions associated with shocked gas, no shocked regions in the intruder galaxy NGC 7318B, and a sharp boundary between shocks and star formation. We conclude that star formation is inhibited substantially, if not entirely, in the shock region. Attributing those H II regions projected against the shock to the intruder, we find a lopsided distribution of star formation in this galaxy, reminiscent of pileup regions in models of interacting galaxies. The Hα luminosities imply mass outputs, star formation rates, and efficiencies similar to nearby star-forming regions. Two large knots are an exception to this, being comparable in stellar output to the prolific 30 Doradus region. We also examine Stephan's Quintet in the context of compact galaxy group evolution, as a paradigm for intermittent star formation histories in the presence of a rich, X-ray-emitting intra-group medium. All spectra are provided as supplemental materials.

AB - We present a Gemini-GMOS spectroscopic study of Hubble Space Telescope (HST)-selected Hα-emitting regions in Stephan's Quintet (HCG 92), a nearby compact galaxy group, with the aim of disentangling the processes of shock-induced heating and star formation in its intra-group medium. The ≈40 sources are distributed across the system, but most densely concentrated in the ∼kiloparsec-long shock region. Their spectra neatly divide them into narrow- and broad-line emitters, and we decompose the latter into three or more emission peaks corresponding to spatial elements discernible in HST imaging. The emission-line ratios of the two populations of Hα-emitters confirm their nature as H II regions (90% of the sample) or molecular gas heated by a shock front propagating at ≲300 km s-1. Their redshift distribution reveals interesting three-dimensional structure with respect to gas-phase baryons, with no H II regions associated with shocked gas, no shocked regions in the intruder galaxy NGC 7318B, and a sharp boundary between shocks and star formation. We conclude that star formation is inhibited substantially, if not entirely, in the shock region. Attributing those H II regions projected against the shock to the intruder, we find a lopsided distribution of star formation in this galaxy, reminiscent of pileup regions in models of interacting galaxies. The Hα luminosities imply mass outputs, star formation rates, and efficiencies similar to nearby star-forming regions. Two large knots are an exception to this, being comparable in stellar output to the prolific 30 Doradus region. We also examine Stephan's Quintet in the context of compact galaxy group evolution, as a paradigm for intermittent star formation histories in the presence of a rich, X-ray-emitting intra-group medium. All spectra are provided as supplemental materials.

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Konstantopoulos IS, Appleton PN, Guillard P, Trancho G, Cluver ME, Bastian N et al. Shocks and star formation in Stephan's quintet. I. Gemini spectroscopy of Hα-Bright knots. Astrophysical Journal. 2014 Mar 20;784(1). 1. https://doi.org/10.1088/0004-637X/784/1/1