Photometry and spectroscopy of the classical nova V339 Del (Nova Del 2013) in the first month after outburst

In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 43, no. 3

D. Chochol - S. Shugarov - T. Pribulla - I. Volkov

Detaily:

Rok, strany: 2014, 330 - 337

Kľúčové slová:

novae, photometry, spectroscopy

URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2014/Vol_43/No_3/pp330-337_abstract.html

Full text

O článku:

The V and B light curves of the classical nova V339 Del, discovered on August 14, 2013, are presented. The V light curve of the nova was used to estimate the times of decline from brightness maximum V = 4.4 mag, reached on August 16.47, 2013, as t_2,V = 10 days, t_3,V = 18 days, so it can be classified as a fast nova. We determined the basic parameters of the nova: absolute magnitude at maximum M_V,max = -8.70±0.03, interstellar extinction E(B-V) = 0.184±0.035 and distance d = 3.2±0.3 kpc. The echelle spectroscopy of the nova obtained on August 15 and 17, 2013 with the 0.6-m Cassegrain telescope at the Stará Lesná Observatory is discussed.

Ako citovať:

ISO 690:

Chochol, D., Shugarov, S., Pribulla, T., Volkov, I. 2014. Photometry and spectroscopy of the classical nova V339 Del (Nova Del 2013) in the first month after outburst. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 43, no.3, pp. 330-337. 1335-1842.

APA:

Chochol, D., Shugarov, S., Pribulla, T., Volkov, I. (2014). Photometry and spectroscopy of the classical nova V339 Del (Nova Del 2013) in the first month after outburst. Contributions of the Astronomical Observatory Skalnaté Pleso, 43(3), 330-337. 1335-1842.