The orbital period of the dwarf nova AF Camelopardalis

Details The orbital period of the dwarf nova AF Camelopardalis The orbital period of the dwarf nova AF Camelopardalis

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aj.....97.1176s&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 97, April 1989, p. 1176-1183.

Astronomy and Astrophysics

Astronomy

4

Dwarf Novae, Stellar Orbits, Astronomical Photometry, Cataclysmic Variables, H Beta Line, H Gamma Line, Periodic Variations

Scientific paper

Time-resolved optical spectroscopy of the dwarf nova AF Cam for 4.5 hr during a decline from outburst reveals that the orbital period is relatively long (5-6 hr). CCD photometry at quiescence also supports this finding. This rules out the previously observed 67-76 min modulations (evident in IR photometric measurements at quiescence and optical photometry at outburst) as orbital in nature.

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