Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-02T19:21:15.419Z Has data issue: false hasContentIssue false
  • English
  • Français

The First Systematic Multi-wavelength Survey of Extragalactic Supernova Remnants

Published online by Cambridge University Press:  29 January 2014

I. Leonidaki ,
P. Boumis  and
A. Zezas
I. Leonidaki
Affiliation:
Institute of Astronomy, Astrophysics, Space Applications & Remote Sensing, National Observatory of Athens, I. Metaxa & Vas. Pavlou St., Palaia Penteli GR-15236 Athens, Greece email: [email protected], [email protected]
P. Boumis
Affiliation:
Institute of Astronomy, Astrophysics, Space Applications & Remote Sensing, National Observatory of Athens, I. Metaxa & Vas. Pavlou St., Palaia Penteli GR-15236 Athens, Greece email: [email protected], [email protected]
A. Zezas
Affiliation:
University of Crete, Physics Department & Institute of Theoretical & Computational Physics, 71003 Heraklion, Crete, Greece Foundation for Research and Technology-Hellas, 71110 Heraklion, Crete, Greece Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA email: [email protected], [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.

We present the largest sample of multi-wavelength Supernova Remnants (SNRs) in six nearby galaxies, based on Chandra archival data and deep optical narrow-band Hα and [Sii] images as well as spectroscopic observations. We have identified 37 X-ray selected thermal SNRs, 30 of which are new identifications and ~ 400 optical SNRs, for 67 of which we spectroscopically verified their shock-excited nature. We discuss the properties of the X-ray/optically detected SNRs in different types of galaxies and hence different environments, in order to address their dependence on their Interstellar Medium (ISM). We also discuss the SNR populations in the context of the star formation rate of their host galaxies. We cross-correlate parameters of the optically detected SNRs with parameters of coincident X-ray emitting SNRs in order to understand their evolution and investigate possible selection effects.

Keywords

supernova remnantsISMstar formationgalaxies
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S296: Supernova Environmental Impacts , January 2013 , pp. 222 - 225
Copyright
Copyright © International Astronomical Union 2014 

References

Blair, W. P. & Long, K. S. 2004, ApJS, 155, 101Google Scholar
Boumis, P., Xilouris, E. M., Alikakos, J., Christopoulou, P. E., Mavromatakis, F., Katsiyannis, A. C., & Goudis, C. D. 2009, A&A, 499, 789Google Scholar
Charles, P. A. & Seward, F. D. 1995, Exploring the X-ray Universe (Cambridge Univ. Press)Google Scholar
Condon, J. J. & Yin, Q. F. 1990, ApJ, 357, 97CrossRefGoogle Scholar
de Vaucoulers, G., de Vaucoulers, A., Corwin, H. G., Buta, R. J., Paturel, G., & Fouque, P. 1995, Third Reeference Catalog of Bright Galaxies, Springer, New YorkGoogle Scholar
Fesen, R. A. & Milisavljevic, D. 2010, AJ, 140, 1163Google Scholar
Garcia-Lario, P., Manchado, A., Riera, A., Mampaso, A., & Pottasch, S. R. 1991, A&A, 249, 223Google Scholar
Green, D. A. 2009, Bulletin of the Astronomical Society of India 37 45. (See: arxiv:0905.3699)Google Scholar
Leonidaki, I., Zezas, A., & Boumis, P. 2010, ApJ, 725, 842CrossRefGoogle Scholar
Leonidaki, I., Boumis, P., & Zezas, A. 2013, MNRAS, 429, 189Google Scholar
Mathewson, D. S. & Clarke, J. N. 1973, ApJ, 180, 725CrossRefGoogle Scholar
Reach, W. T., Rho, J., Tappe, A., Pannuti, T. G., Brogan, C. L., Churchwell, E. B., Meade, M. R., Babler, B., Indebetouw, R., & Whitney, B. A. 2006, AJ, 131, 1479Google Scholar
Reynolds, S. P., Borkowski, K. J., Green, D. A., Hwang, U., Harrus, I., & Petre, R. 2009, ApJ, 695, 149Google Scholar
Sabbadin, F., Minello, S., & Bianchini, A. 1977, A&A, 60, 147Google Scholar
Slane, P., Smith, R. K., Hughes, J. P., & Petre, R. 2002, ApJ, 564, 284Google Scholar
Stupar, M. & Parker, Q. A. 2009, MNRAS, 394, 1791Google Scholar