Nova-like varible V603 Aquilae in 1999

Автор(и)

  • A. V. Baklanov Department of Astronomy, Odessa National University, Україна
  • I. L. Andronov Department of Astronomy, Odessa National University, Україна
  • E. P. Pavlenko Crimean Astrophysical Observatory, Україна

DOI:

https://doi.org/10.18524/1810-4215.2003.16.96933

Ключові слова:

Stars, binary, cataclysmic, nova-like, superhumps, stars, individual, V603 Aql.

Анотація

We perform the CCD (R) photometry of the nova-like variable V603 Aquilae (Nova Aquilae 1918) during 7 nights in 1999. The star showed quasi-periodic oscillations (QPO) with cycles ranging from 03035 to about 09055, and ”positive” superhumps with a photometric period of 014443? days. The ”A- scalegram” analysis shows evidence for QPOs with an effective period P : 17.6 minutes and an amplitude of 23 mmag.

 

Посилання

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2017-03-27

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