In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 54, no. 2
E. Pavlenko - S. Shugarov - T. Kato - O. Antonyuk - A. Sosnovskij - Ju. Babina - A. Shchurova - K. Isogai - A. Sklyanov - A. Gutaev - R. Zhuchkov - P. Dubovsky - K. Petrik - J. Hambsch
Detaily:
Rok, strany: 2024, 117 - 127
Jazyk: eng
Kľúčové slová:
accretion, accretion disks, cataclysmic variables, stars: dwarf novae, stars: individual: V1006 Cyg
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2024/Vol_54/No_2/pp117-127_abstract.html
O článku:
We present a result of the multi-longitude campaign on a photometric investigation of the SU UMa-type dwarf nova in the period gap, V1006 Cyg in 2023. It displayed a long-lasted standstill (a feature of Z Cam-type stars) terminated by a long outburst (a feature of IW And stars). The long outburst did not have superhumps (a feature of SS Cyg-type stars) but showed orbital 0.09837(22) d periodicity instead. Color-color diagrams indicate that layers of the disk of different temperatures contribute to the total radiation of the system. In particular, a large contribution from the innermost hot layers is detected in quiescence.
Ako citovať:
ISO 690:
Pavlenko, E., Shugarov, S., Kato, T., Antonyuk, O., Sosnovskij, A., Babina, J., Shchurova, A., Isogai, K., Sklyanov, A., Gutaev, A., Zhuchkov, R., Dubovsky, P., Petrik, K., Hambsch, J. 2024. V1006 Cyg: SU UMa-type dwarf nova in the period gap that wobbles between subclasses. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 54, no.2, pp. 117-127. 1335-1842. DOI: https://doi.org/10.31577/caosp.2024.54.2.117
APA:
Pavlenko, E., Shugarov, S., Kato, T., Antonyuk, O., Sosnovskij, A., Babina, J., Shchurova, A., Isogai, K., Sklyanov, A., Gutaev, A., Zhuchkov, R., Dubovsky, P., Petrik, K., Hambsch, J. (2024). V1006 Cyg: SU UMa-type dwarf nova in the period gap that wobbles between subclasses. Contributions of the Astronomical Observatory Skalnaté Pleso, 54(2), 117-127. 1335-1842. DOI: https://doi.org/10.31577/caosp.2024.54.2.117
O vydaní:
Vydavateľ: Astronomical Institute, Slovak Academy of Sciences
Publikované: 1. 2. 2024
Verejná licencia:
