In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 43, no. 3
D.yu. Tsvetkov - N.n. Pavlyuk - I.m. Volkov - S.yu. Shugarov
Details:
Year, pages: 2014, 351 - 356
Keywords:
supernovae, photometry
Original source URL: http://www.astro.sk/caosp/Eedition/Abstracts/2014/Vol_43/No_3/pp351-356_abstract.html
About article:
The program of CCD photometric monitoring of bright supernovae (SNe) is carried out at 0.4 — 1.0 meter telescopes of the Sternberg Astronomical Institute, Crimean Astrophysical Observatory and Stará Lesná Observatory since 1998. We have observed more than 250 SNe of different types. We present the results of observations of SNe Ia 2003du, 2009nr and 2011fe, type IIb SNe 2008ax, 2011dh, type II SNe 2004ek and 2005kd and discuss physical parameters of the explosions.
How to cite:
ISO 690:
Tsvetkov, D., Pavlyuk, N., Volkov, I., Shugarov, S. 2014. Photometric monitoring of bright supernovae. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 43, no.3, pp. 351-356. 1335-1842.
APA:
Tsvetkov, D., Pavlyuk, N., Volkov, I., Shugarov, S. (2014). Photometric monitoring of bright supernovae. Contributions of the Astronomical Observatory Skalnaté Pleso, 43(3), 351-356. 1335-1842.