Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-20T06:26:29.261Z Has data issue: false hasContentIssue false
  • English
  • Français

Through the kaleidoscope: star formation the host galaxies of radio-AGN

Published online by Cambridge University Press:  25 July 2014

Marios Karouzos ,
Myungshin Im ,
Markos Trichas ,
Tomo Goto ,
Matt Malkan ,
Angel Ruiz ,
Yiseul Jeon  and
the AKARI NEP team
Marios Karouzos
Affiliation:
CEOU - Astronomy Program, Department of Physics & Astronomy, Seoul National University, Gwanak-gu, Seoul, Korea email: [email protected]
Myungshin Im
Affiliation:
CEOU - Astronomy Program, Department of Physics & Astronomy, Seoul National University, Gwanak-gu, Seoul, Korea email: [email protected]
Markos Trichas
Affiliation:
EADS Astrium Ltd., Gunnels Wood Road, Stevenage SG1 2AS, UK
Tomo Goto
Affiliation:
Dark Cosmology Centre, Niels Bohr Institute University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen, Denmark
Matt Malkan
Affiliation:
Division of Astronomy and Astrophysics, 3-714 UCLA, LA CA 90005-1547, USA
Angel Ruiz
Affiliation:
Inter-University Centre for Astronomy and Astrophysics (IUCAA), Post Bag 4, Ganeshkhind, 411 077 Pune, India
Yiseul Jeon
Affiliation:
CEOU - Astronomy Program, Department of Physics & Astronomy, Seoul National University, Gwanak-gu, Seoul, Korea email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

There exist strong evidence supporting the co-evolution of central supermassive black holes and their host galaxies; however it is still under debate how such a relation comes about and whether it is relevant for all or only a subset of galaxies. A rich multi-wavelength dataset is available for the North Ecliptic Pole field, most notably surveyed by the AKARI infrared space telescope. We investigate the star-formation properties of the host galaxies of radio-AGN together with the radio feedback mechanism, potentially responsible for the eventual quenching of star formation. Using broadband SED modelling, the nuclear and host galaxy components of these sources are studied as a function of their radio luminosity. Here we present results concerning the AGN content of the radio sources in this field, while offering evidence supporting a “maintenance” type of feedback from powerful radio-jets.

Keywords

galaxies: activegalaxies: evolutiongalaxies: jetsradio continuum: galaxiesinfrared: galaxies
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S304: Multiwavelength AGN Surveys and Studies , October 2013 , pp. 323 - 326
Copyright
Copyright © International Astronomical Union 2014 

References

Arnouts, S., Cristiani, S., Moscardini, L., et al. 1999, MNRAS, 310, 540CrossRefGoogle Scholar
Bell, E. F. 2003, ApJ, 586, 794Google Scholar
Bicknell, G. V., Sutherland, R. S., van Breugel, W. J. M., et al. 2000, ApJ, 540, 678CrossRefGoogle Scholar
Croton, D. J., Springel, V., White, S. D. M., et al. 2006, MNRAS, 365, 11Google Scholar
Karouzos, M., Im, M., Trichas, M., et al. 2014a, ApJ, 784, 137Google Scholar
Elbaz, D., Dickinson, M., Hwang, H. S., et al. 2011, A&A, 533, A119Google Scholar
Fabian, A. C. 2012, Ann. Rev. Astron. Astrophys., 50, 455Google Scholar
Gaibler, V., Khochfar, S., Krause, M., & Silk, J. 2012, MNRAS, 425, 438Google Scholar
Hwang, N., Lee, M. G., Lee, H. M., et al. 2007, ApJS, 172, 583Google Scholar
Ilbert, O., Arnouts, S., McCracken, H. J., et al. 2006, A&A, 457, 841Google Scholar
Kormendy, J. & Ho, L. C. 2013, Ann. Rev. Astron. Astrophys., 51, 511Google Scholar
Mauch, T. & Sadler, E. M. 2007, MNRAS, 375, 931Google Scholar
McNamara, B. R., Nulsen, P. E. J., Wise, M. W., et al. 2005, Nature, 433, 45Google Scholar
Morganti, R., Frieswijk, W., Oonk, et al. 2013, A&A, 552, L4Google Scholar
Murakami, H., Baba, H., Barthel, P., et al. 2007, PASJ, 59, 369Google Scholar
Rowan-Robinson, M., Babbedge, T., Oliver, S., et al. 2008, MNRAS, 386, 697Google Scholar
Ruiz, A., Miniutti, G., Panessa, F., & Carrera, F. J. 2010, A&A, 515, A99Google Scholar
Seymour, N., McHardy, I. M., & Gunn, K. F. 2004, MNRAS, 352, 131CrossRefGoogle Scholar
Stern, D., Assef, R. J., Benford, D. J., et al. 2012, ApJ, 753, 30Google Scholar
Strazzullo, V., Pannella, M., Owen, F. N., et al. 2010, ApJ, 714, 1305Google Scholar
Trichas, M., Green, P. J., Silverman, J. D., et al. 2012, ApJS, 200, 17CrossRefGoogle Scholar
Wagner, A. Y. & Bicknell, G. V. 2011, ApJ, 728, 29CrossRefGoogle Scholar
White, G. J., Pearson, C., Braun, R., et al. 2010, A&A, 517, A54Google Scholar
Wright, E. L., Eisenhardt, P. R. M., Mainzer, A. K., et al. 2010, AJ, 140, 1868Google Scholar