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Magnetars: the explosive character of a small class of strongly magnetized neutron stars

Published online by Cambridge University Press:  07 August 2014

Nanda Rea
Nanda Rea*
Affiliation:
Institut de Ciències de l'Espai (CSIC–IEEC), Campus UAB, Facultat de Ciències, Torre C5-parell, E-08193 Barcelona, Spain email: [email protected] Astronomical Institute “Anton Pannekoek”, University of Amsterdam, Postbus 94249, NL-1090 GE Amsterdam, the Netherlands
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Abstract

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I will review our current knowledge on the most magnetic objects in the Universe, a small sample of neutron stars called magnetars. The powerful persistent high energy emission and the flares from these strongly magnetized (1015 Gauss) neutron stars are providing crucial information about the physics involved at these extremes conditions, reserving us many unexpected surprises.

Keywords

neutron starsmagnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S302: Magnetic Fields throughout Stellar Evolution , August 2013 , pp. 429 - 434
Copyright
Copyright © International Astronomical Union 2014 

References

Baade, W & Zwicky, F. 1934 Physical Review 46, 76–77Google Scholar
Baring, M. G. & Harding, A. K., 1998, ApJ, 507, L55Google Scholar
Camilo, F., et al. 2006, Nature 442, 892–895Google Scholar
Chandrasekhar, S. 1931, ApJ 74, 81Google Scholar
Duncan, R. C. & Thompson, C 1992, ApJ 392, L9–L13Google Scholar
Espinoza, C. M., Lyne, A. G., Kramer, M., Manchester, R. N., & Kaspi, V. M., 2011, ApJ 741, L13Google Scholar
Gavriil, F. P., Gonzalez, M. E., Gotthelf, E. V., Kaspi, V. M., Livingstone, M. A., & Woods, P. M. 2008, Science 319, 1802–1805CrossRefGoogle Scholar
Goldreich, P. & Julian, W. H., 1969, ApJ, 157, 869Google Scholar
Harding, A. K. & Lai, D. 2006, RPPh, 69, 2631Google Scholar
Hewish, A., Bell, S. J., Pilkington, J. D. H., Scott, P. F., & Collins, R. A. 1968, Nature 217, 709–713Google Scholar
Halpern, J. P.; Gotthelf, E. V.; Camilo, F.; Seward, F. D. 2007, ApJ 665 1304Google Scholar
Keane, E. F. & McLaughlin, M. A. 2011, BASI, 39, 333Google Scholar
Kumar, H. S. & Safi-Harb, S. 2008, ApJ 678, L43–L46CrossRefGoogle Scholar
Levin, L., et al. 2010 ApJ 721, L33–L37Google Scholar
Manchester, R. N., Hobbs, G. B., Teoh, A., & Hobbs, M. 2005, AJ 129, 1993CrossRefGoogle Scholar
Mereghetti, S. 2008, A&AR, 15 225Google Scholar
Mereghetti, S. 2011, APSS, High-Energy Emission from Pulsars and their Systems, Eds. Rea, N. & Torres, D. F., Springer-Verlag BerlinGoogle Scholar
Nobili, L.; Turolla, R.; Zane, S. 2008, MNRAS, 386, 1527Google Scholar
Pons, J. A. & Rea, N. 2011, ApJ 750, L6Google Scholar
Rea, N., Zane, S., Lyutikov, M., & Turolla, R. 2007, Ap&SS 308, 61Google Scholar
Rea, N.; Zane, S., Turolla, R., Lyutikov, M., & Götz, D. 2008, ApJ 686, 1245Google Scholar
Rea, N., Esposito, P., Turolla, R., Israel, G. L., Zane, S., Stella, L., Mereghetti, S., Tiengo, A., Gotz, D., Gogus, E., & Kouveliotou, C. 2010, Science 330, 944Google Scholar
Rea, N. & Esposito, P. 2011, APSS, High-Energy Emission from Pulsars and their Systems, Eds. Rea, N. & Torres, D. F., Springer-Verlag BerlinGoogle Scholar
Rea, N., Pons, J. A., Torres, D. F., & Turolla, R., 2012a, ApJ, 748, L12CrossRefGoogle Scholar
Rea, N., et al. 2012b, ApJ, 754, 27Google Scholar
Ruderman, M. A. & Sutherland, P. G., 1975, ApJ, 196, 51Google Scholar
Tendulkhar, S.et al. 2012, ApJ submittedGoogle Scholar
Thompson, C., Lyutikov, M., Kulkarni, S. R. 2002, ApJ 574, 332Google Scholar
Thompson, C. & Duncan, R. C. 1993, ApJ 408, 194Google Scholar
Turolla, R. 2009, ASSL, 357, 141Google Scholar
Viganó, D. & Pons, J. A. 2012, MNRAS, 425, 2487CrossRefGoogle Scholar