In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 51, no. 2
S.v. Antipin - A.m. Zubareva - A.a. Belinski - M.a. Burlak - N.p. Ikonnikova - K.l. Malanchev - M.v. Kornilov - E.o. Mishin
Details:
Year, pages: 2021, 132 - 137
Language: eng
Keywords:
stars, photometry, dwarf novae, ZTF18abdlzhd
Original source URL: http://www.astro.sk/caosp/Eedition/Abstracts/2021/Vol_51/No_2/pp132-137_abstract.html
About article:
We carried out a search for unknown dwarf novae in a public data release of the Zwicky Transient Facility survey and suspected that the object ZTF18abdlzhd is a SU UMa-type star. Performed multicolor CCD observations permit us to follow its fading from an outburst in August and an entire superoutburst in October 2020. The duration of the superoutburst is 13 days. We detected superhumps with period P = 0.06918(3) d that are characteristic of UGSU type stars.
How to cite:
ISO 690:
Antipin, S., Zubareva, A., Belinski, A., Burlak, M., Ikonnikova, N., Malanchev, K., Kornilov, M., Mishin, E. 2021. New SU UMa-type star ZTF18abdlzhd in the Zwicky Transient Facility data. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 51, no.2, pp. 132-137. 1335-1842. DOI: https://doi.org/10.31577/caosp.2021.51.2.132
APA:
Antipin, S., Zubareva, A., Belinski, A., Burlak, M., Ikonnikova, N., Malanchev, K., Kornilov, M., Mishin, E. (2021). New SU UMa-type star ZTF18abdlzhd in the Zwicky Transient Facility data. Contributions of the Astronomical Observatory Skalnaté Pleso, 51(2), 132-137. 1335-1842. DOI: https://doi.org/10.31577/caosp.2021.51.2.132
About edition:
Publisher: Astronomical Institute, Slovak Academy of Sciences
Published: 1. 6. 2021
Rights:
