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| Query : 2020RNAAS...4..142S |
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
| Number of rows : 3 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | RX J0045.4+4154 | No* | 00 45 28.80 | +41 54 10.1 | ~ | 263 | 1 | |||||
| 2 | OGLE 2016-NOVA-1 | No* | 05 09 58.3903831759 | -71 39 52.714123608 | 16.0 | 17.0 | 17.38 | ~ | 87 | 0 | ||
| 3 | NAME LMC | G | 05 23 34.6 | -69 45 22 | 0.4 | ~ | 19090 | 0 |
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