A close quasar pair in a disk-disk galaxy merger at z = 2.17.


Journal

Nature
ISSN: 1476-4687
Titre abrégé: Nature
Pays: England
ID NLM: 0410462

Informations de publication

Date de publication:
04 2023
Historique:
received: 13 09 2022
accepted: 26 01 2023
medline: 7 4 2023
entrez: 5 4 2023
pubmed: 6 4 2023
Statut: ppublish

Résumé

Galaxy mergers produce pairs of supermassive black holes (SMBHs), which may be witnessed as dual quasars if both SMBHs are rapidly accreting. The kiloparsec (kpc)-scale separation represents a physical regime sufficiently close for merger-induced effects to be important

Identifiants

pubmed: 37020007
doi: 10.1038/s41586-023-05766-6
pii: 10.1038/s41586-023-05766-6
doi:

Types de publication

Journal Article Research Support, Non-U.S. Gov't Research Support, U.S. Gov't, Non-P.H.S.

Langues

eng

Sous-ensembles de citation

IM

Pagination

45-49

Subventions

Organisme : NASA
ID : GO2-23099X
Pays : United States

Commentaires et corrections

Type : CommentIn

Informations de copyright

© 2023. The Author(s), under exclusive licence to Springer Nature Limited.

Références

Hopkins, P. F., Hernquist, L., Cox, T. J. & Kereš, D. A cosmological framework for the co-evolution of quasars, supermassive black holes, and elliptical galaxies. I. Galaxy mergers and quasar activity. Astrophys. J. Suppl. Ser. 175, 356–389 (2008).
doi: 10.1086/524362
Bogdanović, T., Miller, M. C. & Blecha, L. Electromagnetic counterparts to massive black-hole mergers. Living Rev. Relativ. 25, 3 (2022).
doi: 10.1007/s41114-022-00037-8 pubmed: 35767150 pmcid: 9232481
Richards, G. T. et al. The Sloan Digital Sky Survey Quasar Survey: quasar luminosity function from data release 3. Astron. J. 131, 2766–2787 (2006).
doi: 10.1086/503559
Madau, P. & Dickinson, M. Cosmic star-formation history. Annu. Rev. Astro. Astrophys. 52, 415–486 (2014).
doi: 10.1146/annurev-astro-081811-125615
Schneider, D. P. et al. The Sloan Digital Sky Survey Quasar Catalog. V. Seventh data release. Astron. J. 139, 2360–2373 (2010).
doi: 10.1088/0004-6256/139/6/2360
Hwang, H.-C., Shen, Y., Zakamska, N. & Liu, X. Varstrometry for off-nucleus and dual subkiloparsec agn (VODKA): methodology and initial results with gaia dr2. Astrophys. J. 888, 73 (2020).
doi: 10.3847/1538-4357/ab5c1a
Shen, Y. et al. A hidden population of high-redshift double quasars unveiled by astrometry. Nat. Astron. 5, 569–574 (2021).
doi: 10.1038/s41550-021-01323-1
Barnacka, A., Geller, M. J., Dell’Antonio, I. P. & Benbow, W. Strong gravitational lensing as a tool to investigate the structure of jets at high energies. Astrophys. J. 788, 139 (2014).
doi: 10.1088/0004-637X/788/2/139
Chang, K. & Refsdal, S. Flux variations of qso 0957  561 a, b and image splitting by stars near the light path. Nature 282, 561–564 (1979).
doi: 10.1038/282561a0
Wambsganss, J. & Paczynski, B. Expected color variations of the gravitationally microlensed qso 2237+0305. Astron. J. 102, 864–868 (1991).
doi: 10.1086/115916
Pooley, D., Blackburne, J. A., Rappaport, S., Schechter, P. L. & Fong, W.-f A strong X-ray flux ratio anomaly in the quadruply lensed quasar PG 1115+080. Astrophys. J. 648, 67–72 (2006).
doi: 10.1086/505860
Zezas, A., Alonso-Herrero, A. & Ward, M. J. Searching for X-ray luminous starburst galaxies. Astrophys. Space Sci. 276, 601–607 (2001).
doi: 10.1023/A:1017526118945
Kellermann, K. I., Sramek, R., Schmidt, M., Shaffer, D. B. & Green, R. VLA observations of objects in the Palomar Bright Quasar Survey. Astron. J. 98, 1195–1207 (1989).
doi: 10.1086/115207
Sluse, D., Hutsemékers, D., Courbin, F., Meylan, G. & Wambsganss, J. Microlensing of the broad line region in 17 lensed quasars. Astron. Astrophys. 544, A62 (2012).
doi: 10.1051/0004-6361/201219125
Contreras-Santos, A. et al. Galaxy pairs in The Three Hundred simulations: a study on the performance of observational pair-finding techniques. Mon. Not. R. Astron. Soc. 515, 5375–5388 (2022).
doi: 10.1093/mnras/stac2127
Shapley, A. E. Physical properties of galaxies from z = 2 to 4. Annu. Rev. Astron. Astrophys. 49, 525–580 (2011).
doi: 10.1146/annurev-astro-081710-102542
Ding, X., Silverman, J. D. & Onoue, M. Opening the era of quasar-host studies at high redshift with JWST. Astrophys. J. Lett. 939, L28 (2022).
doi: 10.3847/2041-8213/ac9c02
Shangguan, J. et al. Chandra X-ray and Hubble Space Telescope imaging of optically selected kiloparsec-scale binary active galactic nuclei. II. Host galaxy morphology and AGN activity. Astrophys. J. 823, 50 (2016).
doi: 10.3847/0004-637X/823/1/50
Shields, G. A. et al. LBQS 0103-2753: a binary quasar in a major merger. Astrophys. J. 744, 151 (2012).
doi: 10.1088/0004-637X/744/2/151
Inada, N. et al. The sloan digital sky survey quasar lens search. ii. Statistical lens sample from the third data release. Astron. J. 135, 496–511 (2008).
doi: 10.1088/0004-6256/135/2/496
Schechter, P. L. et al. First lensed quasar systems from the vst-atlas survey: one quad, two doubles, and two pairs of lensless twins. Astron. J. 153, 219 (2017).
doi: 10.3847/1538-3881/aa6899
Anguita, T. et al. The strong lensing insights into the dark energy survey (strides) 2016 follow-up campaign – ii. New quasar lenses from double component fitting. Mon. Not. R. Astron. Soc. 480, 5017–5028 (2018).
Lemon, C. A., Auger, M. W., McMahon, R. G. & Ostrovski, F. Gravitationally lensed quasars in Gaia – II. Discovery of 24 lensed quasars. Mon. Not. R. Astron. Soc. 479, 5060–5074 (2018).
doi: 10.1093/mnras/sty911
Lemon, C. et al. The strong lensing insights into the dark energy survey (strides) 2017/2018 follow-up campaign: discovery of 10 lensed quasars and 10 quasar pairs. Mon. Not. R. Astron. Soc. 494, 3491–3511 (2020).
doi: 10.1093/mnras/staa652
Tang, S. et al. Optical spectroscopy of dual quasar candidates from the Subaru HSC-SSP program. Astrophys. J. 922, 83 (2021).
doi: 10.3847/1538-4357/ac1ff0
Yue, M., Fan, X., Yang, J. & Wang, F. A candidate kiloparsec-scale quasar pair at z = 5.66. Astrophys. J. Lett. 921, L27 (2021).
doi: 10.3847/2041-8213/ac31a9
Lemon, C. et al. J1721+8842: a gravitationally lensed binary quasar with a proximate damped lyman-α absorber. Astron. Astrophys. 657, A113 (2022).
doi: 10.1051/0004-6361/202142138
Kochanek, C. S., Falco, E. E. & Muñoz, J. A. Why quasar pairs are binary quasars and not gravitational lenses. Astrophys. J. 510, 590–596 (1999).
doi: 10.1086/306594
Hennawi, J. F. et al. Binary quasars at high redshift. I. 24 New quasar pairs at z ∼ 3-4. Astrophys. J. 719, 1672–1692 (2010).
doi: 10.1088/0004-637X/719/2/1672
Hennawi, J. F., Prochaska, J. X., Cantalupo, S. & Arrigoni-Battaia, F. Quasar quartet embedded in giant nebula reveals rare massive structure in distant universe. Science 348, 779–783 (2015).
doi: 10.1126/science.aaa5397 pubmed: 25977547
Peng, C. Y., Ho, L. C., Impey, C. D. & Rix, H.-W. Detailed decomposition of galaxy images. II. Beyond axisymmetric models. Astron. J. 139, 2097–2129 (2010).
doi: 10.1088/0004-6256/139/6/2097

Auteurs

Yu-Ching Chen (YC)

Department of Astronomy, University of Illinois at Urbana-Champaign, Urbana, IL, USA.
National Center for Supercomputing Applications, University of Illinois at Urbana-Champaign, Champaign, IL, USA.

Xin Liu (X)

Department of Astronomy, University of Illinois at Urbana-Champaign, Urbana, IL, USA. xinliuxl@illinois.edu.
National Center for Supercomputing Applications, University of Illinois at Urbana-Champaign, Champaign, IL, USA. xinliuxl@illinois.edu.

Adi Foord (A)

Kavli Institute of Particle Astrophysics and Cosmology, Stanford University, Stanford, CA, USA.

Yue Shen (Y)

Department of Astronomy, University of Illinois at Urbana-Champaign, Urbana, IL, USA.
National Center for Supercomputing Applications, University of Illinois at Urbana-Champaign, Champaign, IL, USA.

Masamune Oguri (M)

Center for Frontier Science, Chiba University, Chiba, Japan.
Department of Physics, Graduate School of Science, Chiba University, Chiba, Japan.

Nianyi Chen (N)

McWilliams Center for Cosmology, Department of Physics, Carnegie Mellon University, Pittsburgh, PA, USA.

Tiziana Di Matteo (T)

McWilliams Center for Cosmology, Department of Physics, Carnegie Mellon University, Pittsburgh, PA, USA.
NSF AI Planning Institute for Physics of the Future, Carnegie Mellon University, Pittsburgh, PA, USA.
OzGrav-Melbourne, Australian Research Council Centre of Excellence for Gravitational Wave Discovery, Melbourne, Victoria, Australia.

Miguel Holgado (M)

McWilliams Center for Cosmology, Department of Physics, Carnegie Mellon University, Pittsburgh, PA, USA.

Hsiang-Chih Hwang (HC)

School of Natural Sciences, Institute for Advanced Study, Princeton, NJ, USA.

Nadia Zakamska (N)

Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA.

Classifications MeSH