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Autor:
Russell, David M., Bramich, D. M., Lewis, F., AlMannaei, A., Qaissieh, T. Al, Qasim, A. Al, Yazeedi, A. Al, Baglio, M. C., Bernardini, F., Elgalad, N., Gabuya, A., Lasota, J. P., Palado, A., Roche, P., Shivkumar, H., Udrescu, S., Zhang, G.
Disc instability models predict that for X-ray binaries in quiescence, there should be a brightening of the optical flux prior to an X-ray outburst. Tracking the X-ray variations of X-ray binaries in quiescence is generally not possible, so optical m
Externí odkaz:
http://arxiv.org/abs/1903.04519