Deductions from the Indication of Eclipses of Nova V1493 Aql

Details Deductions from the Indication of Eclipses of Nova V1493 Aql Deductions from the Indication of Eclipses of Nova V1493 Aql

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap%26ss.304..317f&link_type=abstract

Astrophysics and Space Science, Volume 304, Issue 1-4, pp. 317-319

Astronomy and Astrophysics

Astrophysics

2

Nova, Wind

Scientific paper

Our mainly R band photometry of V1493 Aql (1999) during its outburst, indicates periodic variations with a period of 0.156 days, seen only 5 days after the maximum in V. This period can be orbital. The light curve indicates in addition, the presence of a faint eclipse like feature. We try to explain its extremely low amlitude, as being due to the eclipse of an expanded white dwarf component of the binary below an optically thick wind. We discuss what conditions would be required for such an interpretation to work.

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