Optical observations of ‘hot’ novae returning to quiescence-Reference-Cited by-同舟云学术

Optical observations of ‘hot’ novae returning to quiescence

Published:2018-08-24 Issue:4 Volume:480 Page:4489-4504
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Zemko P¹,Ciroi S¹,Orio M²³,Odendaal A⁴,Shugarov S⁵⁶,Barsukova E⁷,Bianchini A³,Cracco V¹,Gabdeev M⁷,Goranskij V⁵,Tofflemire B²,Valeev A F⁷⁸,Katysheva N⁵

Affiliation:

1. Department of Physics and Astronomy, Università di Padova, vicolo dell’Osservatorio 3, I-35122 Padova, Italy

2. Department of Astronomy, University of Wisconsin, 475 N. Charter Street, Madison, WI 53704, USA

3. INAF - Osservatorio di Padova, vicolo dell’ Osservatorio 5, I-35122 Padova, Italy

4. Department of Physics, University of the Free State, 9300 Bloemfontein, South Africa

5. Sternberg Astrophysical Institute, Lomonosov Moscow University, Universitetsky Ave., 13, Moscow 119992, Russia

6. Astronomical Institute of the Slovak Academy of Sciences, Tatranská Lomnica, 059 60, The Slovak Republic

7. Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnij Arkhyz, Karachai-Cherkesia 369167, Russia

8. Kazan Federal University, Kremlevskaya 18, 420008 Kazan, Russia

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/480/4/4489/25539410/sty2061.pdf

Reference121 articles.

1. A pre-outburst signal in the long-term optical light curve of the recurrent nova RS Ophiuchi

2. The Spectral Evolution of V382 Velorum (Nova Vela 1999)

3. Multiwavelength observations of V407 Lupi (ASASSN-16kt) – a very fast nova erupting in an intermediate polar

4. The Detection of a 3.5 hr Period in the Classical Nova Velorum 1999 (V382 Vel) and the Long-Term Behavior of the Nova Light Curve

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