Paschen-α emission in the gravitationally lensed galaxy SMM

Casey Papovich, Gregory Rudnick, Jane R. Rigby, Christopher N A Willmer, J. D T Smith, Steven L. Finkelstein, Eiichi Egami, Marcia J Rieke

Research output: Contribution to journalArticle

13 Citations (Scopus)

Abstract

We report the detection of the Paα emission line in the z = 2.515 galaxy SMM J163554.2+661225 using Spitzer spectroscopy. SMM J163554.2+661225 is a submillimeter-selected infrared-luminous galaxy maintaining a high star formation rate (SFR), with no evidence of an active galactic nucleus from optical or infrared spectroscopy, nor X-ray emission. This galaxy is lensed gravitationally by the cluster Abell 2218, making it accessible to Spitzer spectroscopy. We measure a line luminosity, L(Paα) = (2.05 0.33) × 1042 erg s-1, corrected for gravitational lensing. Comparing the Hα and Paα luminosities, we derive a nebular extinction, A(V) = 3.6 0.4mag. The dust-corrected luminosity, L(Paα) = (2.57 0.43) × 1042 erg s-1, corresponds to an ionization rate, Q 0 = (1.6 0.3) × 1055 γs-1. The instantaneous SFR is ψ = 171 28 M ȯ yr-1, assuming a Salpeter-like initial mass function from 0.1 to 100 M ȯyr-1. The total IR luminosity derived using 70, 450, and 850μm data is LIR = (5-10) × 1011 L , corrected for gravitational lensing. This corresponds to ψ = 90-180 M yr-1, where the upper range is consistent with that derived from the Paα luminosity. While the L(8 μm)/L(Paα) ratio is consistent with the extrapolated relation observed in local galaxies and star-forming regions, the rest-frame 24μm luminosity is significantly lower with respect to local galaxies of comparable Paα luminosity. Thus, SMM J163554.2+661225 arguably lacks a warmer dust component (TD ∼ 70 K), which is associated with deeply embedded star formation, and which contrasts with local galaxies with comparable SFRs. Rather, the starburst in SMM J163554.2+661225 is consistent with star-forming local galaxies with intrinsic luminosities, L IR 1010 L , but "scaled up" by a factor of 10-100.

Original languageEnglish (US)
Pages (from-to)1506-1518
Number of pages13
JournalAstrophysical Journal
Volume704
Issue number2
DOIs
StatePublished - 2009

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luminosity
galaxies
star formation rate
erg
dust
spectroscopy
stars
infrared spectroscopy
active galactic nuclei
star formation
extinction
ionization
rate
x rays

Keywords

  • Galaxies: formation
  • Galaxies: high-redshift
  • Galaxies: starburst
  • Infrared: galaxies

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Papovich, C., Rudnick, G., Rigby, J. R., Willmer, C. N. A., Smith, J. D. T., Finkelstein, S. L., ... Rieke, M. J. (2009). Paschen-α emission in the gravitationally lensed galaxy SMM. Astrophysical Journal, 704(2), 1506-1518. https://doi.org/10.1088/0004-637X/704/2/1506

Paschen-α emission in the gravitationally lensed galaxy SMM. / Papovich, Casey; Rudnick, Gregory; Rigby, Jane R.; Willmer, Christopher N A; Smith, J. D T; Finkelstein, Steven L.; Egami, Eiichi; Rieke, Marcia J.

In: Astrophysical Journal, Vol. 704, No. 2, 2009, p. 1506-1518.

Research output: Contribution to journalArticle

Papovich, C, Rudnick, G, Rigby, JR, Willmer, CNA, Smith, JDT, Finkelstein, SL, Egami, E & Rieke, MJ 2009, 'Paschen-α emission in the gravitationally lensed galaxy SMM', Astrophysical Journal, vol. 704, no. 2, pp. 1506-1518. https://doi.org/10.1088/0004-637X/704/2/1506
Papovich C, Rudnick G, Rigby JR, Willmer CNA, Smith JDT, Finkelstein SL et al. Paschen-α emission in the gravitationally lensed galaxy SMM. Astrophysical Journal. 2009;704(2):1506-1518. https://doi.org/10.1088/0004-637X/704/2/1506
Papovich, Casey ; Rudnick, Gregory ; Rigby, Jane R. ; Willmer, Christopher N A ; Smith, J. D T ; Finkelstein, Steven L. ; Egami, Eiichi ; Rieke, Marcia J. / Paschen-α emission in the gravitationally lensed galaxy SMM. In: Astrophysical Journal. 2009 ; Vol. 704, No. 2. pp. 1506-1518.
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N2 - We report the detection of the Paα emission line in the z = 2.515 galaxy SMM J163554.2+661225 using Spitzer spectroscopy. SMM J163554.2+661225 is a submillimeter-selected infrared-luminous galaxy maintaining a high star formation rate (SFR), with no evidence of an active galactic nucleus from optical or infrared spectroscopy, nor X-ray emission. This galaxy is lensed gravitationally by the cluster Abell 2218, making it accessible to Spitzer spectroscopy. We measure a line luminosity, L(Paα) = (2.05 0.33) × 1042 erg s-1, corrected for gravitational lensing. Comparing the Hα and Paα luminosities, we derive a nebular extinction, A(V) = 3.6 0.4mag. The dust-corrected luminosity, L(Paα) = (2.57 0.43) × 1042 erg s-1, corresponds to an ionization rate, Q 0 = (1.6 0.3) × 1055 γs-1. The instantaneous SFR is ψ = 171 28 M ȯ yr-1, assuming a Salpeter-like initial mass function from 0.1 to 100 M ȯyr-1. The total IR luminosity derived using 70, 450, and 850μm data is LIR = (5-10) × 1011 L ⊙, corrected for gravitational lensing. This corresponds to ψ = 90-180 M ⊙ yr-1, where the upper range is consistent with that derived from the Paα luminosity. While the L(8 μm)/L(Paα) ratio is consistent with the extrapolated relation observed in local galaxies and star-forming regions, the rest-frame 24μm luminosity is significantly lower with respect to local galaxies of comparable Paα luminosity. Thus, SMM J163554.2+661225 arguably lacks a warmer dust component (TD ∼ 70 K), which is associated with deeply embedded star formation, and which contrasts with local galaxies with comparable SFRs. Rather, the starburst in SMM J163554.2+661225 is consistent with star-forming local galaxies with intrinsic luminosities, L IR 1010 L ⊙, but "scaled up" by a factor of 10-100.

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