VODKA-JWST: A 3.8 kpc Dual Quasar at Cosmic Noon in a Powerful Starburst Galaxy with JWST/MIRI Integral Field Unit

Dual quasars—two active supermassive black holes at galactic scales—represent crucial objects for studying the impact of galaxy mergers and quasar activity on the star formation rate (SFR) within their host galaxies, particularly at cosmic noon when SFR peaks. We present JWST/MIRI mid-infrared integ...

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Vydáno v:The Astrophysical journal Ročník 968; číslo 2; s. 92 - 100
Hlavní autoři: Chen, Yu-Ching, Ishikawa, Yuzo, Zakamska, Nadia L., Liu, Xin, Shen, Yue, Hwang, Hsiang-Chih, Rupke, David, Vayner, Andrey, Gross, Arran C., Liu, Weizhe, Wylezalek, Dominika, Veilleux, Sylvain, Bertemes, Caroline, Diachenko, Nadiia, Sankar, Swetha
Médium: Journal Article
Jazyk:angličtina
Vydáno: Philadelphia The American Astronomical Society 01.06.2024
IOP Publishing
Témata:
Active galactic nuclei
Aromatic hydrocarbons
Black holes
Depletion
Double quasars
Galaxies
Galaxy mergers
Galaxy mergers & collisions
Infrared astronomy
Integral field spectroscopy
James Webb Space Telescope
Luminosity
Molecular gases
Polycyclic aromatic hydrocarbons
Quasars
Red shift
Spectroscopy
Star & galaxy formation
Star formation
Star formation rate
Starburst galaxies
Stars
Stars & galaxies
Stellar mass
Supermassive black holes
Vodka
Water outflow
ISSN:0004-637X, 1538-4357
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Abstract Dual quasars—two active supermassive black holes at galactic scales—represent crucial objects for studying the impact of galaxy mergers and quasar activity on the star formation rate (SFR) within their host galaxies, particularly at cosmic noon when SFR peaks. We present JWST/MIRI mid-infrared integral field spectroscopy of J074922.96+225511.7, a dual quasar with a projected separation of 3.8 kpc at a redshift z = 2.17. We detect spatially extended [Fe ii ] 5.34 μ m and polycyclic aromatic hydrocarbon (PAH) 3.3 μ m emissions from the star formation activity in its host galaxy. We derive the SFR of 10 3.0±0.2 M ⊙ yr −1 using PAH 3.3 μ m, which is 5 times higher than that derived from the knee of the infrared luminosity function for galaxies at z ∼ 2. While the SFR of J0749+2255 agrees with that of star-forming galaxies of comparable stellar mass at the same redshifts, its molecular gas content falls short of expectations based on the molecular Kennicutt–Schmidt law. This discrepancy may result from molecular gas depletion due to the longer elevated stage of star formation, even after the molecular gas reservoir is depleted. We do not observe any quasar-driven outflow that impacts PAH and [Fe ii ] in the host galaxy based on the spatially resolved maps. From the expected flux in PAH-based star formation, the [Fe ii ] line likely originates from the star-forming regions in the host galaxy. Our study highlights the extreme stardust nature of J0749+2255, indicating a potential connection between the dual quasar phase and intense star formation activities.
AbstractList Dual quasars—two active supermassive black holes at galactic scales—represent crucial objects for studying the impact of galaxy mergers and quasar activity on the star formation rate (SFR) within their host galaxies, particularly at cosmic noon when SFR peaks. We present JWST/MIRI mid-infrared integral field spectroscopy of J074922.96+225511.7, a dual quasar with a projected separation of 3.8 kpc at a redshift z = 2.17. We detect spatially extended [Fe ii ] 5.34 μ m and polycyclic aromatic hydrocarbon (PAH) 3.3 μ m emissions from the star formation activity in its host galaxy. We derive the SFR of 10 ^3.0±0.2 M _⊙ yr ^−1 using PAH 3.3 μ m, which is 5 times higher than that derived from the knee of the infrared luminosity function for galaxies at z ∼ 2. While the SFR of J0749+2255 agrees with that of star-forming galaxies of comparable stellar mass at the same redshifts, its molecular gas content falls short of expectations based on the molecular Kennicutt–Schmidt law. This discrepancy may result from molecular gas depletion due to the longer elevated stage of star formation, even after the molecular gas reservoir is depleted. We do not observe any quasar-driven outflow that impacts PAH and [Fe ii ] in the host galaxy based on the spatially resolved maps. From the expected flux in PAH-based star formation, the [Fe ii ] line likely originates from the star-forming regions in the host galaxy. Our study highlights the extreme stardust nature of J0749+2255, indicating a potential connection between the dual quasar phase and intense star formation activities.
Dual quasars—two active supermassive black holes at galactic scales—represent crucial objects for studying the impact of galaxy mergers and quasar activity on the star formation rate (SFR) within their host galaxies, particularly at cosmic noon when SFR peaks. We present JWST/MIRI mid-infrared integral field spectroscopy of J074922.96+225511.7, a dual quasar with a projected separation of 3.8 kpc at a redshift z = 2.17. We detect spatially extended [Fe ii ] 5.34 μ m and polycyclic aromatic hydrocarbon (PAH) 3.3 μ m emissions from the star formation activity in its host galaxy. We derive the SFR of 10 3.0±0.2 M ⊙ yr −1 using PAH 3.3 μ m, which is 5 times higher than that derived from the knee of the infrared luminosity function for galaxies at z ∼ 2. While the SFR of J0749+2255 agrees with that of star-forming galaxies of comparable stellar mass at the same redshifts, its molecular gas content falls short of expectations based on the molecular Kennicutt–Schmidt law. This discrepancy may result from molecular gas depletion due to the longer elevated stage of star formation, even after the molecular gas reservoir is depleted. We do not observe any quasar-driven outflow that impacts PAH and [Fe ii ] in the host galaxy based on the spatially resolved maps. From the expected flux in PAH-based star formation, the [Fe ii ] line likely originates from the star-forming regions in the host galaxy. Our study highlights the extreme stardust nature of J0749+2255, indicating a potential connection between the dual quasar phase and intense star formation activities.
Dual quasars—two active supermassive black holes at galactic scales—represent crucial objects for studying the impact of galaxy mergers and quasar activity on the star formation rate (SFR) within their host galaxies, particularly at cosmic noon when SFR peaks. We present JWST/MIRI mid-infrared integral field spectroscopy of J074922.96+225511.7, a dual quasar with a projected separation of 3.8 kpc at a redshift z = 2.17. We detect spatially extended [Fe ii] 5.34 μm and polycyclic aromatic hydrocarbon (PAH) 3.3 μm emissions from the star formation activity in its host galaxy. We derive the SFR of 103.0±0.2M⊙ yr−1 using PAH 3.3 μm, which is 5 times higher than that derived from the knee of the infrared luminosity function for galaxies at z ∼ 2. While the SFR of J0749+2255 agrees with that of star-forming galaxies of comparable stellar mass at the same redshifts, its molecular gas content falls short of expectations based on the molecular Kennicutt–Schmidt law. This discrepancy may result from molecular gas depletion due to the longer elevated stage of star formation, even after the molecular gas reservoir is depleted. We do not observe any quasar-driven outflow that impacts PAH and [Fe ii] in the host galaxy based on the spatially resolved maps. From the expected flux in PAH-based star formation, the [Fe ii] line likely originates from the star-forming regions in the host galaxy. Our study highlights the extreme stardust nature of J0749+2255, indicating a potential connection between the dual quasar phase and intense star formation activities.
Author Rupke, David
Shen, Yue
Hwang, Hsiang-Chih
Vayner, Andrey
Ishikawa, Yuzo
Bertemes, Caroline
Zakamska, Nadia L.
Liu, Weizhe
Chen, Yu-Ching
Wylezalek, Dominika
Diachenko, Nadiia
Veilleux, Sylvain
Liu, Xin
Gross, Arran C.
Sankar, Swetha
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  surname: Ishikawa
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  organization: Johns Hopkins University Department of Physics and Astronomy, Bloomberg Center, Baltimore, MD 21218, USA
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  givenname: Nadia L.
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  surname: Zakamska
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  givenname: Xin
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  organization: University of Illinois at Urbana-Champaign Center for Artificial Intelligence Innovation, 1205 West Clark Street, Urbana, IL 61801, USA
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  surname: Shen
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  organization: University of Illinois at Urbana-Champaign Department of Astronomy, Urbana, IL 61801, USA
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  givenname: David
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  surname: Rupke
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  organization: Department of Physics, Rhodes College, 2000 N. Parkway, Memphis, TN 38112, USA
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  surname: Gross
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  organization: University of Illinois at Urbana-Champaign Department of Astronomy, Urbana, IL 61801, USA
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  orcidid: 0000-0003-3762-7344
  surname: Liu
  fullname: Liu, Weizhe
  organization: University of Arizona Department of Astronomy, Steward Observatory, Tucson, AZ 85719, USA
– sequence: 11
  givenname: Dominika
  orcidid: 0000-0003-2212-6045
  surname: Wylezalek
  fullname: Wylezalek, Dominika
  organization: Zentrum für Astronomie der Universität Heidelberg, Astronomisches Rechen-Institut, Mönchhofstr 12-14, D-69120 Heidelberg, Germany
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  givenname: Sylvain
  orcidid: 0000-0002-3158-6820
  surname: Veilleux
  fullname: Veilleux, Sylvain
  organization: University of Maryland Department of Astronomy and Joint Space-Science Institute, College Park, MD 20742, USA
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  orcidid: 0000-0002-6948-1485
  surname: Bertemes
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  givenname: Swetha
  orcidid: 0000-0002-4419-8325
  surname: Sankar
  fullname: Sankar, Swetha
  organization: Johns Hopkins University Department of Physics and Astronomy, Bloomberg Center, Baltimore, MD 21218, USA
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SubjectTerms Active galactic nuclei
Aromatic hydrocarbons
Black holes
Depletion
Double quasars
Galaxies
Galaxy mergers
Galaxy mergers & collisions
Infrared astronomy
Integral field spectroscopy
James Webb Space Telescope
Luminosity
Molecular gases
Polycyclic aromatic hydrocarbons
Quasars
Red shift
Spectroscopy
Star & galaxy formation
Star formation
Star formation rate
Starburst galaxies
Stars
Stars & galaxies
Stellar mass
Supermassive black holes
Vodka
Water outflow
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