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Gamma-ray emission from pulsar/massive-star binaries

Published online by Cambridge University Press:  21 October 2010

Gustavo E. Romero
Gustavo E. Romero*
Affiliation:
Instituto Argentino de Radioastronomía (IAR, CCT La Plata, CONICET), C.C.5, (1894) Villa Elisa, Buenos Aires, Argentina email: [email protected] Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque s/n, 1900 La Plata, Argentina email: [email protected]
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Abstract

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I present a review of the main phenomenological properties at high energies related to massive gamma-ray binaries and I discuss some aspects of pulsar models for these objects.

Keywords

Radiation mechanisms: non-thermalstars: neutronstars: early-typestars: windsoutflowsgamma rays: observationsgamma rays: theory
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 126 - 130
Copyright
Copyright © International Astronomical Union 2010

References

Abdo, A. A. (Fermi coll.) 2009, ApJ (Lett.), in press (arXiv:0907.4307)Google Scholar
Acciari, V. A. (VERITAS coll.) 2009, ApJ, 700, 1034CrossRefGoogle Scholar
Albert, J. et al. (MAGIC coll.) 2006, Science 312, 1771Google Scholar
Aharonian, F. A. et al. (HESS col.) 2005a, A&A 442, 1Google Scholar
Aharonian, F. A. et al. (HESS col.) 2005b, Science 309, 746Google Scholar
Aharonian, F. A. et al. (HESS col.) 2006, A&A 460, 743Google Scholar
Berezinskii, V.S., Castagnoli, C. and Galeotti, P. M. 1986, ApJ 301, 235Google Scholar
Bogovalov, S. V. & Kelner, S. R. 2005, Astron. Rep 49, 57CrossRefGoogle Scholar
Bosch-Ramon, V., Paredes, J. M., Romero, G. E., & Ribó, M. 2006, A&A 459, L25Google Scholar
Bosch-Ramon, V., Khangulyan, D., & Aharonian, F. A. 2008, A&A 489, L21Google Scholar
Casares, J., et al. , 2005, MNRAS 364, 899CrossRefGoogle Scholar
Cheng, K. S. & Ruderman, M. 1989, ApJ 337, L77CrossRefGoogle Scholar
Dermer, C. D. & Boettcher, M. 2006, ApJ 643, 1081Google Scholar
Dhawan, V., Mioduszewski, A., & Rupen, M., 2006, in Proc. of the VI Microquasar Workshop, Como-2006Google Scholar
Dubus, W., 2006, A&A 456, 801Google Scholar
Khangulyan, D., Hnatic, S., Aharonian, F.A., & Bogovalov, S. 2007, MNRAS 380, 320Google Scholar
Khangulyan, D., Aharonian, F. A., & Bosch-Ramon, V. 2008, MNRAS 383, 467Google Scholar
Johnston, S., Ball, L., Wang, N., & Manchester, R. N. 2005, MNRAS 358, 1069Google Scholar
Maraschi, L. & Treves, A. 1981, MNRAS 194, 1Google Scholar
Orellana, M., Romero, G. E., Pellizza, L. J., & Vidrih, S. 2007, A&A 465, 703Google Scholar
Paredes, J. M., Martí, J., Ribó, M., & Massi, M., 2000, Science 288, 2340Google Scholar
Romero, G. E., et al. 2001, A&A 376, 599Google Scholar
Romero, G. E., Christiansen, H. R., & Orellana, M., 2005, ApJ 632, 1093Google Scholar
Romero, G. E., Okazaki, A. T., Orellana, M., & Owocki, S. P. 2007, A&A 474, 15Google Scholar
Sguera, V., et al. 2009, ApJ 697, 1194Google Scholar
Skilton, J. L., et al. 2009, MNRAS, in press (arXiv:0906.3411)Google Scholar
Tavani, M. & Arons, J. 1997, ApJ 477, 439Google Scholar
Tavani, M., Arons, J. & Kaspi, V. 1994, ApJ (Lett.) 433, L37Google Scholar