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2020RNAAS...4..142S - Research Notes of the AAS, 4, 142 (2020/August-0)

Similarities between the X-Ray Light Curves of the 2016 and 2020 Eruptions of the Recurrent Nova LMC 1968.

SCHWARZ G.J., PAGE K.L., KUIN P.M. and DARNLEY M.J.

Abstract (from CDS):

The latest eruption of the recurrent nova LMC 1968 was extensively observed by Swift with its X-ray Telescope instrument. A comparison with the Swift data set from the 2016 eruption shows that the X-ray evolution was remarkably similar just as the evolution of the optical photometry and spectroscopy was similar during previously observed eruptions. The only difference is a surprising decrease in the recurrence time. LMC 1968 is only the second nova for which Swift has observed the entire X-ray evolution more than once. At 50 kpc, it is close enough to be extensively observed in its next eruption.

Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.

Journal keyword(s): Recurrent novae - X-ray binary stars - X-ray transient sources

Simbad objects: 3

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