V404 CYG/GS 2023+338: Monitoring in the Optical with Robotic Telescopes of the MASTER Global Network during the 2015 Superburst
- Authors: Lipunov V.M.1,2, Kuznetsov A.S.1, Gorbovskoy E.S.1, Kornilov V.G.1, Tyurina N.V.1, Vladimirov V.V.1, Krushinskiy V.V.3, Zalozhnykh I.S.3, Vlasenko D.M.1,2, Zimnukhov D.S.1, Balanutsa P.V.1, Gabovich A.1,4, Shakura N.I.1, Giovanelli F.5, Titarchuk L.G.1,6, Buckley D.A.7, Gress O.1,8, Budnev N.8, Rebolo R.9, Serra-Ricart M.8, Tlatov A.G.10, Senik V.A.1, Yurkov V.V.10, Ershova O.7, Grinshpun V.G.2, Ishmukhametova Y.V.8
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Affiliations:
- Sternberg Astronomical Institute
- Physics Department
- Kourovka Astronomical Observatory
- Blagoveshchensk State Pedagogical University
- Institute Nationale di Astrofisica
- Ferrara University
- South African Astronomical Observatory (SAAO)
- Irkutsk State University, Applied Physics Institute
- Instituto de Astrofísica de Canarias
- Kislovodsk Solar Station of the Main (Pulkovo) Observatory
- Issue: Vol 63, No 7 (2019)
- Pages: 534-549
- Section: Article
- URL: https://journals.rcsi.science/1063-7729/article/view/192954
- DOI: https://doi.org/10.1134/S1063772919070059
- ID: 192954
Cite item
Abstract
2070 unique, homogeneous photometric and polarization observations of the microquasar in a binary system with a black hole V404 Cyg/GS2023+338 obtained in 2015 with the MASTER global network of robotic telescopes (16 robotic telescopes located at eight points on the Earth in Russia, Spain, South Africa, and Argentina) are presented. MASTER was the first telescope network to obtain optical observations of the microquasar after its gamma-ray outburst in 2015. Observations were carried out from 18:34:09 UT on June 15, 2015 until December 2015 in four polarizations and in the four standard BV RI filters. The paper presents the results of these observations and a comparative analysis of optical and X-ray data. The observations confirm the previously discovered super-long delays of the optical radiation relative to the X-ray outbursts. Possible mechanisms causing the delay in the optical variations relative to the X-ray variations are discussed. Variability of the optical polarization discovered earlier is confirmed another similar episode reported.
About the authors
V. M. Lipunov
Sternberg Astronomical Institute; Physics Department
Author for correspondence.
Email: lipunov2007@gmail.com
Russian Federation, Moscow, 119991; Moscow, 119234
A. S. Kuznetsov
Sternberg Astronomical Institute
Email: lipunov2007@gmail.com
Russian Federation, Moscow, 119991
E. S. Gorbovskoy
Sternberg Astronomical Institute
Email: lipunov2007@gmail.com
Russian Federation, Moscow, 119991
V. G. Kornilov
Sternberg Astronomical Institute
Email: lipunov2007@gmail.com
Russian Federation, Moscow, 119991
N. V. Tyurina
Sternberg Astronomical Institute
Email: lipunov2007@gmail.com
Russian Federation, Moscow, 119991
V. V. Vladimirov
Sternberg Astronomical Institute
Email: lipunov2007@gmail.com
Russian Federation, Moscow, 119991
V. V. Krushinskiy
Kourovka Astronomical Observatory
Email: lipunov2007@gmail.com
Russian Federation, Ekaterinburg, 620000
I. S. Zalozhnykh
Kourovka Astronomical Observatory
Email: lipunov2007@gmail.com
Russian Federation, Ekaterinburg, 620000
D. M. Vlasenko
Sternberg Astronomical Institute; Physics Department
Email: lipunov2007@gmail.com
Russian Federation, Moscow, 119991; Moscow, 119234
D. S. Zimnukhov
Sternberg Astronomical Institute
Email: lipunov2007@gmail.com
Russian Federation, Moscow, 119991
P. V. Balanutsa
Sternberg Astronomical Institute
Email: lipunov2007@gmail.com
Russian Federation, Moscow, 119991
A. Gabovich
Sternberg Astronomical Institute; Blagoveshchensk State Pedagogical University
Email: lipunov2007@gmail.com
Russian Federation, Moscow, 119991; Blagoveshchensk, 675000
N. I. Shakura
Sternberg Astronomical Institute
Email: lipunov2007@gmail.com
Russian Federation, Moscow, 119991
F. Giovanelli
Institute Nationale di Astrofisica
Email: lipunov2007@gmail.com
Italy, Roma
L. G. Titarchuk
Sternberg Astronomical Institute; Ferrara University
Email: lipunov2007@gmail.com
Russian Federation, Moscow, 119991; Ferrara
D. A. H. Buckley
South African Astronomical Observatory (SAAO)
Email: lipunov2007@gmail.com
South Africa, Cape Town
O. Gress
Sternberg Astronomical Institute; Irkutsk State University, Applied Physics Institute
Email: lipunov2007@gmail.com
Russian Federation, Moscow, 119991; Irkutsk, 664003
N. Budnev
Irkutsk State University, Applied Physics Institute
Email: lipunov2007@gmail.com
Russian Federation, Irkutsk, 664003
R. Rebolo
Instituto de Astrofísica de Canarias
Email: lipunov2007@gmail.com
Spain, La Laguna, Tenerife
M. Serra-Ricart
Irkutsk State University, Applied Physics Institute
Email: lipunov2007@gmail.com
Russian Federation, Irkutsk, 664003
A. G. Tlatov
Kislovodsk Solar Station of the Main (Pulkovo) Observatory
Email: lipunov2007@gmail.com
Russian Federation, Kislovodsk, 357700
V. A. Senik
Sternberg Astronomical Institute
Email: lipunov2007@gmail.com
Russian Federation, Moscow, 119991
V. V. Yurkov
Kislovodsk Solar Station of the Main (Pulkovo) Observatory
Email: lipunov2007@gmail.com
Russian Federation, Kislovodsk, 357700
O. Ershova
South African Astronomical Observatory (SAAO)
Email: lipunov2007@gmail.com
South Africa, Cape Town
V. G. Grinshpun
Physics Department
Email: lipunov2007@gmail.com
Russian Federation, Moscow, 119234
Yu. V. Ishmukhametova
Irkutsk State University, Applied Physics Institute
Email: lipunov2007@gmail.com
Russian Federation, Irkutsk, 664003
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