PAH Emission and Star Formation in the Host of the [FORMULA][F]z~2.56[/F][/FORMULA] Cloverleaf QSO

  • Lutz D
  • Sturm E
  • Tacconi L
  • et al.
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Abstract

We report the first detection of the 6.2micron and 7.7micron infrared `PAH' emission features in the spectrum of a high redshift QSO, from the Spitzer-IRS spectrum of the Cloverleaf lensed QSO (H1413+117, z~2.56). The ratio of PAH features and rest frame far-infrared emission is the same as in lower luminosity star forming ultraluminous infrared galaxies and in local PG QSOs, supporting a predominantly starburst nature of the Cloverleaf's huge far-infrared luminosity (5.4E12 Lsun, corrected for lensing). The Cloverleaf's period of dominant QSO activity (Lbol ~ 7E13 Lsun) is coincident with an intense (star formation rate ~1000 Msun/yr) and short (gas exhaustion time ~3E7yr) star forming event.

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APA

Lutz, D., Sturm, E., Tacconi, L. J., Valiante, E., Schweitzer, M., Netzer, H., … Veilleux, S. (2007). PAH Emission and Star Formation in the Host of the [FORMULA][F]z~2.56[/F][/FORMULA] Cloverleaf QSO. The Astrophysical Journal, 661(1), L25–L28. https://doi.org/10.1086/518537

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