The Orbital Period of the Classical Nova V368 Aquilae

Details The Orbital Period of the Classical Nova V368 Aquilae The Orbital Period of the Classical Nova V368 Aquilae

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1614....1s&link_type=abstract

The Astronomer's Telegram, #1614

Astronomy and Astrophysics

Astronomy

2

Optical, Cataclysmic Variables, Novae

Scientific paper

The Orbital Period of the Classical Nova V368 Aquilae A. W. Shafter, E. Marin (SDSU), and S. R. Warren (U. Minn) Diaz & Bruch (1994, IBVS, 4079) reported the discovery of eclipses in the light curve of V368 Aql (Nova Aquilae 1936 No. 2), and concluded that the orbital period of the nova was 0.34521 d (8.285 hr). As part of a program to study the light curves of eclipsing novae, we obtained time-resolved CCD photometry of V368 Aql on the nights of 2005 September 3, 4, and 5 UT using the Mount Laguna Observatory 1-m reflector.

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