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Multicolour photometry of SS 433

Published online by Cambridge University Press:  30 December 2019

D. Koçak ,
T. İçli  and
K. Yakut Open the ORCID record for K. Yakut [Opens in a new window]
D. Koçak
Affiliation:
Department of Astronomy & Space Sciences, University of Ege, 35100, Bornova–İzmir, Turkey email: dolunay.kocak@gmail.com
T. İçli
Affiliation:
Department of Astronomy & Space Sciences, University of Ege, 35100, Bornova–İzmir, Turkey email: dolunay.kocak@gmail.com
K. Yakut
Affiliation:
Department of Astronomy & Space Sciences, University of Ege, 35100, Bornova–İzmir, Turkey email: dolunay.kocak@gmail.com
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Abstract

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We presented long-term optical observations of the high mass X-ray binary system SS 433 (V1343 Aql) with a black hole component. New observations have been obtained by using the 0.6m telescope at the TÜBİTAK National Observatory (TUG) in B, V, R and I filters. We aim to investigate the long-term photometric behavior of the system.

Keywords

stars:binariesX-rays: binariesstars: individual (SS 433 V1343 Aql)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S346: High-mass X-ray Binaries: Illuminating the Passage from Massive Binaries to Merging Compact Objects , August 2018 , pp. 252 - 254
Copyright
© International Astronomical Union 2019 

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