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Transient X-ray Binaries in the Magellanic Clouds and Milky Way

Published online by Cambridge University Press:  29 August 2019

P. C. Charles ,
D. Buckley ,
D. Mata Sánchez ,
P. Meintjes ,
A. Rajoelimanana  and
L. Townsend
P. C. Charles*
Affiliation:
Dept of Physics & Astronomy, University of Southampton, UK
D. Buckley
Affiliation:
South African Astronomical Observatory, Cape Town, South Africa
D. Mata Sánchez
Affiliation:
Instituto de Astrofísica de Canarias (IAC), La Laguna, Tenerife, Spain
P. Meintjes
Affiliation:
Department of Physics, University of the Free State, Bloemfontein, South Africa
A. Rajoelimanana
Affiliation:
Department of Physics, University of the Free State, Bloemfontein, South Africa
L. Townsend
Affiliation:
Department of Astronomy, University of Cape Town, South Africa
*
email: [email protected]
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Abstract

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This contribution gave three examples of X-ray transients in the Magellanic Clouds and the Milky Way that have been observed as part of the SALT Transients Large Programme. The transients (SMC X-3, MAXI J1957+032 and ASASSN-16oh) have been triggered from both space-based wide-field monitoring facilities (Swift/XRT, MAXI) and ground-based ones (ASASSN, the All Sky Automated Survey for SN), providing insights into the physics of super-Eddington accretion onto neutron stars and white dwarfs, and also into the long-term properties of accreting millisecond X-ray pulsars.

Keywords

Accretionaccretion disksstars: novæcataclysmic variablesX-rays: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S339: Southern Horizons in Time-Domain Astronomy , November 2017 , pp. 127 - 130
Copyright
© International Astronomical Union 2019 

Footnotes

†

Leverhulme Emeritus Fellow

References

Belloni, T. M., Motta, S. E., & Muñoz-Darias, T. 2011, BASI, 39, 409Google Scholar
Campana, S., et al. 1998, A&AR, 8, 279Google Scholar
Charles, P. 2011, ASPC, 447, 19Google Scholar
Coe, M. J., et al. 2009, in: van Loon, J. T. & Oliveira, J. M. (eds.), The Magellanic System: Stars, Gas and Galaxies, Proc. IAUS 256 (CUP, Cambridge, UK), p. 367Google Scholar
Heinke, C. O., et al. 2010, ApJ, 714, 89410.1088/0004-637X/714/1/894CrossRefGoogle Scholar
Kahabka, P, & van den Heuvel, E. P. J. 2006, in: Lewin, W. & van der Klis, M. (eds.), Compact Stellar X-ray Sources (CUP, Cambridge, UK), p. 461CrossRefGoogle Scholar
Kato, M. 2010, AN, 331, 140Google Scholar
Kennea, J. A., et al. 2016, ATel 9362Google Scholar
Maccarone, T.J., Brown, P., & Mukai, K. 2016, ATel 9866Google Scholar
Mata Sánchez, D., et al. 2017, MNRAS, 468, 564CrossRefGoogle Scholar
Mroz, P., et al. 2016, ATel 9867Google Scholar
Reig, P. 2011, ApSS, 332, 1Google Scholar
Townsend, L. J., et al. 2017, MNRAS, 471, 3878CrossRefGoogle Scholar
Wang, Z., et al. 2001, ApJ, 563, L6110.1086/338357CrossRefGoogle Scholar