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The orbital period of Nova Aquilae 1999 No. 2 (V1494 Aql)

Authors :
V. P. Goranskii
E. A. Barsukova
Source :
Astronomy Letters. 29:195-198
Publication Year :
2003
Publisher :
Pleiades Publishing Ltd, 2003.

Abstract

The photometric monitoring of Nova V 1494 Aql at the Sternberg Astronomical Institute and at the Special Astrophysical Observatory in July and September 2002 has confirmed that the star is an eclipsing system. Its orbital period was improved, $$0\mathop .\limits^d 1346141(5)$$ . Light elements and eight mid-eclipse times are given. The light-curve shape suggests that the star is an intermediate polar.

Subjects

Subjects :
Physics
Astrophysics::High Energy Astrophysical Phenomena
Astrophysics::Instrumentation and Methods for Astrophysics
Astronomy
Astronomy and Astrophysics
Nova (laser)
Astrophysics
Orbital period
Intermediate polar
Space and Planetary Science
Observatory
Astrophysics::Solar and Stellar Astrophysics
Astrophysics::Earth and Planetary Astrophysics
Astrophysics::Galaxy Astrophysics

Details

ISSN :
15626873 and 10637737
Volume :
29
Database :
OpenAIRE
Journal :
Astronomy Letters
Accession number :
edsair.doi...........d9aec03aec8f0f3c6ff9258090f435c2

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Authors Abstract Subjects Details