The Molecular Disk in the Cloverleaf Quasar
arXiv:astro-ph/0210529 · doi:10.1086/375050
Abstract
We propose a new interpretation for the CO emitting region of the Cloverleaf (H1413+1143), a gravitationally lensed QSO. We fit a two-galaxy lensing model directly to the IRAM CO(7-6) data rather than to the optical HST image and from the fit we infer that the CO(7-6) source is a disk-like structure with a characteristic radius of Ω_Λ=0.7Ω_{m}=0.3H_{0}=65 {\rm km s^{-1} mpc}^{-1}$), a size similar to that of the CO emitting regions present in nearby starburst ultraluminous infrared galaxies. We therefore suggest that the Cloverleaf contains both an extended rotating molecular starburst disk and a central quasar.
18 pages, 2 figures, accepted for publication in ApJ
References in corpus (3)
- Molecular Gas and Dust at z = 2.6 in SMM J14011+0252: A Strongly Lensed, Ultraluminous Galaxy, Not a Huge, Massive Disk
- Resolved nuclear CO(1-0) emission in APM08279+5255: Gravitational lensing by a naked cusp?
- Hubble Space Telescope Observations of the Gravitationally Lensed Cloverleaf Broad Absorption Line QSO H1413+1143: Imaging Polarimetry and Evidence for Microlensing of a Scattering Region
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- One of Everything: The Breakthrough Listen Exotica Catalog