Abstract
ABSTRACT The V-band CCD photometry of a faint cataclysmic variable 1329-294 revealed its periodic light variations with the most likely period of 3.8 hours. No eclipse was seen. Known characteristics of this system suggest that it is a dwarf nova.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callMore From: Publications of the Astronomical Society of the Pacific
Paper Title
Journal
Date
