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The Galactic distribution of SNRs

Published online by Cambridge University Press:  29 January 2014

D. A. Green
D. A. Green*
Affiliation:
Cavendish Laboratory, 19 J. J. Thomson Ave., Cambridge, CB3 0HE, U.K. email: [email protected]
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Abstract

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It is not straightforward to determine the distribution of supernova remnants (SNRs) in the Galaxy. The two main difficulties are that there are observational selection effects that mean that catalogues of SNRs are incomplete, and distances are not available for most remnants. Here I discuss the selection effects that apply to the latest catalogue of Galactic SNRs. I then compare the observed distribution of ‘bright’ SNRs in Galactic longitude with that expected from models in order to constrain the Galactic distribution of SNRs.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S296: Supernova Environmental Impacts , January 2013 , pp. 188 - 196
Copyright
Copyright © International Astronomical Union 2014 

References

Brogan, C. L., Gaensler, B. M., Gelfand, J. D., Lazendic, J. S., Lazio, T. J. W., Kassim, N. E., & McClure-Griffiths, N. M., 2005, ApJ, 629, L105Google Scholar
Brogan, C. L., Gelfand, J. D., Gaensler, B. M., Kassim, N. E., & Lazio, T. J. W., 2006, ApJ, 639, L25Google Scholar
Bronfman, L., Casassus, S., May, J., & Nyman, L.-Å., 2000, A&A, 358, 521Google Scholar
Case, G. L. & Bhattacharya, D., 1998, ApJ, 504, 761Google Scholar
Carlton, A. K., Borkowski, K. J., Reynolds, S. P., Hwang, U., Petre, R., Green, D. A., Krishnamurthy, K., & Willett, R., 2011, ApJ, 737, L22CrossRefGoogle Scholar
Fürst, E., Reich, W., Reich, P., & Reif, K., 1990, A&AS, 85, 691Google Scholar
Gao, X. Y., Sun, X. H., Han, J. L., Reich, W., Reich, P., & Wielebinski, R., 2011, A&A, 532, A144Google Scholar
Gray, A. D., 1994, MNRAS, 270, 835Google Scholar
Green, D. A., 1984, MNRAS, 209, 449Google Scholar
Green, D. A., 2005, MmSAI, 76, 534Google Scholar
Green, D. A., 2009a, BASI, 37, 45Google Scholar
Green, D. A., 2009b, MNRAS, 399, 177Google Scholar
Green, D. A., 2012, in: Aharonian, F., Hofmann, W. & Rieger, F. (eds), High Energy Gamma-Ray Astronomy, AIP Conference Proceedings, Volume 1505 (American Institute of Physics, Melville, New York), p. 5Google Scholar
Green, D. A., Reynolds, S. P., Borkowski, K. J., Hwang, U., Harrus, I., & Petre, R., 2008, MNRAS, 387, L54CrossRefGoogle Scholar
Hui, C. Y., Seo, K. A., Huang, R. H. H., Trepl, L., Woo, Y. J., Lu, T.-N., Kong, A. K. H., & Walter, F. M., 2012, ApJ, 750, 7Google Scholar
Hurley-Walker, N., et al., 2009, MNRAS, 398, 249Google Scholar
Isobe, T., Feigelson, E. D., Akritas, M. G., & Babu, G. J., 1990, ApJ, 364, 104Google Scholar
Kassim, N. E. & Frail, D. A., 1996, MNRAS, 283, L51CrossRefGoogle Scholar
Lorimer, D. R., et al., 2006, MNRAS, 372, 777Google Scholar
Reich, W., Fürst, E., Reich, P., Junkes, N., 1988, in: Roger, R. S. & Landecker, T. L. (eds), Supernova Remnants and the Interstellar Medium, Proc. IAU Colloquium No. 101 (Cambridge University Press), p. 293Google Scholar
Reich, W., Fürst, E., Reich, P., & Reif, K., 1990, A&AS, 85, 633Google Scholar
Reynolds, S. P., Borkowski, K. J., Green, D. A., Hwang, U., Harrus, I., & Petre, R., 2008, ApJ, 680, L41Google Scholar
Robbins, W. J., Gaensler, B. M., Murphy, T., Reeves, S., & Green, A. J., 2012, MNRAS, 419, 2623CrossRefGoogle Scholar
Stupar, M., Parker, Q. A., & Filipović, M. D., 2011, Ap&SS, 332, 241Google Scholar
Whiteoak, J. B. Z. & Green, A. J., 1996, A&AS, 118, 329Google Scholar
Yusef-Zadeh, F., Shure, M., Wardle, M., & Kassim, N., 2000, ApJ, 540, 842CrossRefGoogle Scholar