Extremely slow nova VI548 Aql

Автор(и)

  • N. Primak Crimean Astrophysical Observatory, Україна
  • E. P. Pavlenko Crimean Astrophysical Observatory, Україна

DOI:

https://doi.org/10.18524/1810-4215.2003.16.97217

Ключові слова:

stars, binary, cataclysmic, individual, V 1548 Aql.

Анотація

The results of VRI CCD photomet-rical observations of extremely slow nova V1548 Aql
(Nova Aql 2001) in Crimean Astrophysical Observatory during 2001 - 2003 years are presented. During the outburst decline in 2001 there were quasi-periodic brightness variations with period about 57 days (or 28 days). There were also color changes during decline. Brightness variations of V 1548 Aql during long periods, behaviour in color diagrams are presented.The behaviour of slow Nova Aquilae 2001=V 1548 Aql is like the behaviour of some slow novas, i.e. V 723 Gas, HR Del, DO Aql.

 

Посилання

Kato T., Takamizawa K.: 2001, IAU Information Bulletin Variable Stars, 5100

Pelt J .: 1992,Irregulary Spaced Data Analysis, Helsinki.

Primak N.V., Pavlenko E.P., Shugarov S.Yu., et al.: 2002, ”Classical Nova Explosions”, Am.Inst.Phys.Conf. Proc., 637, 319.

Stellingwerf R.F.: 1978, ApJ, 224, 953

VSNET - Alert: 2001a, 5876.

VSNET - Alert: 2001b, 5920.

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Опубліковано

2017-03-29

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