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2017MNRAS.471..373K - Mon. Not. R. Astron. Soc., 471, 373-382 (2017/October-2)
Rapid optical variations correlated with X-rays in the 2015 second outburst of V404 Cygni (GS 2023+338).
KIMURA M., KATO T., ISOGAI K., TAK H., SHIDATSU M., ITOH H., TORDAI T., KASAI K., GOFF W., KIYOTA S., PICKARD R.D., MATSUMOTO K., KOJIGUCHI N., SUGIURA Y., YAMADA E., TATSUMI T., MIYASHITA A., DUBOVSKY P.A., KUDZEJ I., DE MIGUEL E., STEIN W.L., MAEDA Y., PAVLENKO E.P., SOSNOVSKIJ A.A., BABINA J.V., COOK L.M. and NOGAMI D.
Abstract (from CDS):
Abstract Copyright: © 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): accretion, accretion disc - black hole physics - binaries: general - stars: individual: V404 Cygni - X-rays: binaries - X-rays: binaries
Errata: erratum vol. 475, p. 3083 (2018)
Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.
Simbad objects: 5
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