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Autor:
Ilya A. Mereminskiy, Yu. A. Dvorkovich, A. V. Prosvetov, A. S. Grebenev, V. S. Knyazeva, S. A. Grebenev, K. D. Ostashenko
Based on long-term SWIFT, RXTE, and MAXI observations of the X-ray novae H1743-322 (IGR J17464-3213) and GX339-4, we have investigated the morphology and classified the light curves of their X-ray outbursts. In particular, we have confirmed the exist
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::afc02933e9c11310ffa6778f86e3687c
http://arxiv.org/abs/2009.09314
http://arxiv.org/abs/2009.09314