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Dust and Cold Gas P...
Dust and Cold Gas Properties of Starburst HyLIRG Quasars at z ∼ 2.5
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- Liu, Feng Yuan (författare)
- Chinese Academy of Sciences,University of Edinburgh
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- Dai, Y. Sophia (författare)
- Chinese Academy of Sciences
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- Omont, A.A. (författare)
- Institut d 'Astrophysique de Paris
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- Liu, Daizhong (författare)
- Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
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- Cox, P. (författare)
- Institut d 'Astrophysique de Paris
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- Neri, R. (författare)
- Institut de Radioastronomie Millimétrique (IRAM)
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- Krips, M. (författare)
- Institut de Radioastronomie Millimétrique (IRAM)
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- Yang, Chentao, 1988 (författare)
- Chalmers tekniska högskola,Chalmers University of Technology
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- Wu, Xue Bing (författare)
- Beijing University of Technology
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- Huang, Jia Sheng (författare)
- Chinese Academy of Sciences,Harvard-Smithsonian Center for Astrophysics
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(creator_code:org_t)
- 2024
- 2024
- Engelska.
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Ingår i: Astrophysical Journal. - 1538-4357 .- 0004-637X. ; 964:2
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https://research.cha... (primary) (free)
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https://research.cha...
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https://doi.org/10.3...
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Abstract
Ämnesord
Stäng
- Some high-z active galactic nuclei (AGNs) are found to reside in extreme star-forming galaxies, such as hyperluminous infrared galaxies (HyLIRGs), with AGN-removed L IR of >1013 L ⊙. In this paper, we report NOEMA observations of six apparent starburst HyLIRGs associated with optical quasars at z ∼ 2-3 in the Stripe 82 field, to study their dust and molecular CO properties. Five out of the six candidates are detected with CO(4-3) or CO(5-4) emission, and four in the 2 mm dust continuum. Based on the linewidth- L CO ( 1 − 0 ) ′ diagnostics, we find that four galaxies are likely unlensed or weakly lensed sources. The molecular gas mass is in the range of μ M H 2 ∼ 0.8 - 9.7 × 10 10 M ⊙ (with α = 0.8 M ⊙ K km s − 1 pc 2 − 1 , where μ is the unknown possible gravitational magnification factor). We fit their spectral energy distributions, after including the observed 2 mm fluxes and upper limits, and estimate their apparent (uncorrected for possible lensing effects) star formation rates (μSFRs) to be ∼400-2500 M ⊙ yr−1, with a depletion time of ∼20-110 Myr. We notice interesting offsets, of ∼10-40 kpc spatially or ∼1000-2000 km s−1 spectroscopically, between the optical quasar and the millimeter continuum or CO emissions. The observed velocity shift is likely related to the blueshifted broad-emission-line region of quasars, though mergers or recoiling black holes are also possible causes, which can explain the spatial offsets and the high intrinsic star formation rates in the HyLIRG quasar systems.
Ämnesord
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
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Liu, Feng Yuan
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Dai, Y. Sophia
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Omont, A.A.
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Liu, Daizhong
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Cox, P.
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Neri, R.
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visa fler...
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Krips, M.
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Yang, Chentao, 1 ...
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Wu, Xue Bing
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Huang, Jia Sheng
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Chalmers tekniska högskola