In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 39, no. 1
D. Chochol - N.a. Katysheva - S.yu. Shugarov - I.m. Volkov
Detaily:
Rok, strany: 2009, 43 - 65
Kľúčové slová:
dwarf novae, photometry, superoutburst
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2009/Vol_39/No_1/pp43-65_abstract.html
O článku:
We present the UBV(RI)C photometry of the dwarf nova Tri 2008 = OT
J023839.1+355648 obtained during its superoutburst started on October 25,
2008. The object can be classified as a WZ Sge-type dwarf nova. The period
of early superhumps 0.05307 days was detected in the first 7 days of the
superoutburst. The period of ordinary superhumps 0.053663 days, detected in
days 8-23 of the superoutburst, is the shortest one among WZ Sge-type
objects. After one month, the dwarf nova returned to its pre-outburst state.
A sudden increase of activity of the object during its quiescent stage was
detected on January 11, 2009.
Ako citovať:
ISO 690:
Chochol, D., Katysheva, N., Shugarov, S., Volkov, I. 2009. CCD photometry of the dwarf nova Trianguli 2008 - a new WZ Sge-type object. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 39, no.1, pp. 43-65. 1335-1842.
APA:
Chochol, D., Katysheva, N., Shugarov, S., Volkov, I. (2009). CCD photometry of the dwarf nova Trianguli 2008 - a new WZ Sge-type object. Contributions of the Astronomical Observatory Skalnaté Pleso, 39(1), 43-65. 1335-1842.