The impact of galaxy interactions on active galactic nucleus activity in zCOSMOS

J. D. Silverman, P. Kampczyk, K. Jahnke, R. Andrae, S. J. Lilly, M. Elvis, F. Civano, V. Mainieri, C. Vignali, G. Zamorani, P. Nair, O. Le Fèvre, L. De Ravel, S. Bardelli, A. Bongiorno, M. Bolzonella, A. Cappi, K. Caputi, C. M. Carollo, T. ContiniG. Coppa, O. Cucciati, S. De La Torre, P. Franzetti, B. Garilli, C. Halliday, G. Hasinger, A. Iovino, C. Knobel, A. M. Koekemoer, K. Kovač, F. Lamareille, J. F. Le Borgne, V. Le Brun, C. Maier, M. Mignoli, R. Pello, E. Pérez-Montero, E. Ricciardelli, Y. Peng, M. Scodeggio, M. Tanaka, L. Tasca, L. Tresse, D. Vergani, E. Zucca, M. Brusa, Nico Cappelluti, A. Comastri, A. Finoguenov, H. Fu, R. Gilli, H. Hao, L. C. Ho, M. Salvato

Research output: Contribution to journalArticle

95 Citations (Scopus)

Abstract

Close encounters between galaxies are expected to be a viable mechanism, as predicted by numerical simulations, by which accretion onto supermassive black holes can be initiated. To test this scenario, we construct a sample of 562 galaxies (M * > 2.5 × 1010 M ) in kinematic pairs over the redshift range 0.25 < z < 1.05 that are more likely to be interacting than a well-matched control sample of 2726 galaxies not identified as being in a pair, both from the zCOSMOS 20k spectroscopic catalog. Galaxies that harbor an active galactic nucleus (AGN) are identified on the basis of their X-ray emission (L 0.5-10 keV > 2 × 1042ergs-1) detected by Chandra. We find a higher fraction of an AGN in galaxies in pairs relative to isolated galaxies of similar stellar mass. Our result is primarily due to an enhancement of AGN activity, by a factor of 1.9 (observed) and 2.6 (intrinsic), for galaxies in pairs of projected separation less than 75kpc and line-of-sight velocity offset less than 500kms-1. This study demonstrates that close kinematic pairs are conducive environments for black hole growth, either indicating a causal physical connection or an inherent relation, such as, to enhanced star formation. In the Appendix, we describe a method for estimating the intrinsic fractions of galaxies (either in pairs or the field) hosting an AGN with confidence intervals, and an excess fraction in pairs. We estimate that 17.8+8.4 -7.4% of all moderate-luminosity AGN activity takes place within galaxies undergoing early stages of interaction that leaves open the question as to what physical processes are responsible for fueling the remaining 80% that may include late-stage mergers.

Original languageEnglish (US)
Article number2
JournalAstrophysical Journal
Volume743
Issue number1
DOIs
StatePublished - Dec 10 2011
Externally publishedYes

Fingerprint

interacting galaxies
active galactic nuclei
kinematics
galaxies
merger
confidence interval
accretion
simulation
refueling
stellar mass
encounters
leaves
line of sight
star formation
confidence
estimating
luminosity
intervals
augmentation
estimates

Keywords

  • galaxies: active
  • galaxies: interactions
  • quasars: general
  • X-rays: galaxies

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Silverman, J. D., Kampczyk, P., Jahnke, K., Andrae, R., Lilly, S. J., Elvis, M., ... Salvato, M. (2011). The impact of galaxy interactions on active galactic nucleus activity in zCOSMOS. Astrophysical Journal, 743(1), [2]. https://doi.org/10.1088/0004-637X/743/1/2

The impact of galaxy interactions on active galactic nucleus activity in zCOSMOS. / Silverman, J. D.; Kampczyk, P.; Jahnke, K.; Andrae, R.; Lilly, S. J.; Elvis, M.; Civano, F.; Mainieri, V.; Vignali, C.; Zamorani, G.; Nair, P.; Le Fèvre, O.; De Ravel, L.; Bardelli, S.; Bongiorno, A.; Bolzonella, M.; Cappi, A.; Caputi, K.; Carollo, C. M.; Contini, T.; Coppa, G.; Cucciati, O.; De La Torre, S.; Franzetti, P.; Garilli, B.; Halliday, C.; Hasinger, G.; Iovino, A.; Knobel, C.; Koekemoer, A. M.; Kovač, K.; Lamareille, F.; Le Borgne, J. F.; Le Brun, V.; Maier, C.; Mignoli, M.; Pello, R.; Pérez-Montero, E.; Ricciardelli, E.; Peng, Y.; Scodeggio, M.; Tanaka, M.; Tasca, L.; Tresse, L.; Vergani, D.; Zucca, E.; Brusa, M.; Cappelluti, Nico; Comastri, A.; Finoguenov, A.; Fu, H.; Gilli, R.; Hao, H.; Ho, L. C.; Salvato, M.

In: Astrophysical Journal, Vol. 743, No. 1, 2, 10.12.2011.

Research output: Contribution to journalArticle

Silverman, JD, Kampczyk, P, Jahnke, K, Andrae, R, Lilly, SJ, Elvis, M, Civano, F, Mainieri, V, Vignali, C, Zamorani, G, Nair, P, Le Fèvre, O, De Ravel, L, Bardelli, S, Bongiorno, A, Bolzonella, M, Cappi, A, Caputi, K, Carollo, CM, Contini, T, Coppa, G, Cucciati, O, De La Torre, S, Franzetti, P, Garilli, B, Halliday, C, Hasinger, G, Iovino, A, Knobel, C, Koekemoer, AM, Kovač, K, Lamareille, F, Le Borgne, JF, Le Brun, V, Maier, C, Mignoli, M, Pello, R, Pérez-Montero, E, Ricciardelli, E, Peng, Y, Scodeggio, M, Tanaka, M, Tasca, L, Tresse, L, Vergani, D, Zucca, E, Brusa, M, Cappelluti, N, Comastri, A, Finoguenov, A, Fu, H, Gilli, R, Hao, H, Ho, LC & Salvato, M 2011, 'The impact of galaxy interactions on active galactic nucleus activity in zCOSMOS', Astrophysical Journal, vol. 743, no. 1, 2. https://doi.org/10.1088/0004-637X/743/1/2
Silverman JD, Kampczyk P, Jahnke K, Andrae R, Lilly SJ, Elvis M et al. The impact of galaxy interactions on active galactic nucleus activity in zCOSMOS. Astrophysical Journal. 2011 Dec 10;743(1). 2. https://doi.org/10.1088/0004-637X/743/1/2
Silverman, J. D. ; Kampczyk, P. ; Jahnke, K. ; Andrae, R. ; Lilly, S. J. ; Elvis, M. ; Civano, F. ; Mainieri, V. ; Vignali, C. ; Zamorani, G. ; Nair, P. ; Le Fèvre, O. ; De Ravel, L. ; Bardelli, S. ; Bongiorno, A. ; Bolzonella, M. ; Cappi, A. ; Caputi, K. ; Carollo, C. M. ; Contini, T. ; Coppa, G. ; Cucciati, O. ; De La Torre, S. ; Franzetti, P. ; Garilli, B. ; Halliday, C. ; Hasinger, G. ; Iovino, A. ; Knobel, C. ; Koekemoer, A. M. ; Kovač, K. ; Lamareille, F. ; Le Borgne, J. F. ; Le Brun, V. ; Maier, C. ; Mignoli, M. ; Pello, R. ; Pérez-Montero, E. ; Ricciardelli, E. ; Peng, Y. ; Scodeggio, M. ; Tanaka, M. ; Tasca, L. ; Tresse, L. ; Vergani, D. ; Zucca, E. ; Brusa, M. ; Cappelluti, Nico ; Comastri, A. ; Finoguenov, A. ; Fu, H. ; Gilli, R. ; Hao, H. ; Ho, L. C. ; Salvato, M. / The impact of galaxy interactions on active galactic nucleus activity in zCOSMOS. In: Astrophysical Journal. 2011 ; Vol. 743, No. 1.
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abstract = "Close encounters between galaxies are expected to be a viable mechanism, as predicted by numerical simulations, by which accretion onto supermassive black holes can be initiated. To test this scenario, we construct a sample of 562 galaxies (M * > 2.5 × 1010 M ⊙) in kinematic pairs over the redshift range 0.25 < z < 1.05 that are more likely to be interacting than a well-matched control sample of 2726 galaxies not identified as being in a pair, both from the zCOSMOS 20k spectroscopic catalog. Galaxies that harbor an active galactic nucleus (AGN) are identified on the basis of their X-ray emission (L 0.5-10 keV > 2 × 1042ergs-1) detected by Chandra. We find a higher fraction of an AGN in galaxies in pairs relative to isolated galaxies of similar stellar mass. Our result is primarily due to an enhancement of AGN activity, by a factor of 1.9 (observed) and 2.6 (intrinsic), for galaxies in pairs of projected separation less than 75kpc and line-of-sight velocity offset less than 500kms-1. This study demonstrates that close kinematic pairs are conducive environments for black hole growth, either indicating a causal physical connection or an inherent relation, such as, to enhanced star formation. In the Appendix, we describe a method for estimating the intrinsic fractions of galaxies (either in pairs or the field) hosting an AGN with confidence intervals, and an excess fraction in pairs. We estimate that 17.8+8.4 -7.4{\%} of all moderate-luminosity AGN activity takes place within galaxies undergoing early stages of interaction that leaves open the question as to what physical processes are responsible for fueling the remaining 80{\%} that may include late-stage mergers.",
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AU - Kampczyk, P.

AU - Jahnke, K.

AU - Andrae, R.

AU - Lilly, S. J.

AU - Elvis, M.

AU - Civano, F.

AU - Mainieri, V.

AU - Vignali, C.

AU - Zamorani, G.

AU - Nair, P.

AU - Le Fèvre, O.

AU - De Ravel, L.

AU - Bardelli, S.

AU - Bongiorno, A.

AU - Bolzonella, M.

AU - Cappi, A.

AU - Caputi, K.

AU - Carollo, C. M.

AU - Contini, T.

AU - Coppa, G.

AU - Cucciati, O.

AU - De La Torre, S.

AU - Franzetti, P.

AU - Garilli, B.

AU - Halliday, C.

AU - Hasinger, G.

AU - Iovino, A.

AU - Knobel, C.

AU - Koekemoer, A. M.

AU - Kovač, K.

AU - Lamareille, F.

AU - Le Borgne, J. F.

AU - Le Brun, V.

AU - Maier, C.

AU - Mignoli, M.

AU - Pello, R.

AU - Pérez-Montero, E.

AU - Ricciardelli, E.

AU - Peng, Y.

AU - Scodeggio, M.

AU - Tanaka, M.

AU - Tasca, L.

AU - Tresse, L.

AU - Vergani, D.

AU - Zucca, E.

AU - Brusa, M.

AU - Cappelluti, Nico

AU - Comastri, A.

AU - Finoguenov, A.

AU - Fu, H.

AU - Gilli, R.

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AU - Salvato, M.

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AB - Close encounters between galaxies are expected to be a viable mechanism, as predicted by numerical simulations, by which accretion onto supermassive black holes can be initiated. To test this scenario, we construct a sample of 562 galaxies (M * > 2.5 × 1010 M ⊙) in kinematic pairs over the redshift range 0.25 < z < 1.05 that are more likely to be interacting than a well-matched control sample of 2726 galaxies not identified as being in a pair, both from the zCOSMOS 20k spectroscopic catalog. Galaxies that harbor an active galactic nucleus (AGN) are identified on the basis of their X-ray emission (L 0.5-10 keV > 2 × 1042ergs-1) detected by Chandra. We find a higher fraction of an AGN in galaxies in pairs relative to isolated galaxies of similar stellar mass. Our result is primarily due to an enhancement of AGN activity, by a factor of 1.9 (observed) and 2.6 (intrinsic), for galaxies in pairs of projected separation less than 75kpc and line-of-sight velocity offset less than 500kms-1. This study demonstrates that close kinematic pairs are conducive environments for black hole growth, either indicating a causal physical connection or an inherent relation, such as, to enhanced star formation. In the Appendix, we describe a method for estimating the intrinsic fractions of galaxies (either in pairs or the field) hosting an AGN with confidence intervals, and an excess fraction in pairs. We estimate that 17.8+8.4 -7.4% of all moderate-luminosity AGN activity takes place within galaxies undergoing early stages of interaction that leaves open the question as to what physical processes are responsible for fueling the remaining 80% that may include late-stage mergers.

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