The orbital period of Nova Aquilae 1999 No. 2 (V1494 Aql)
- 1 March 2003
- journal article
- Published by Pleiades Publishing Ltd in Astronomy Letters
- Vol. 29 (3) , 195-198
- https://doi.org/10.1134/1.1558159
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, $$0mathop .limits^d 1346141(5)$$ . Light elements and eight mid-eclipse times are given. The light-curve shape suggests that the star is an intermediate polar.
Keywords
This publication has 2 references indexed in Scilit:
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- An RR Lyrae Star Survey with Ihe Lick 20-INCH Astrograph II. The Calculation of RR Lyrae Periods by Electronic Computer.The Astrophysical Journal Supplement Series, 1965