Statistical analysis of the long-term visual light curve parameters of dwarf novae

Details Statistical analysis of the long-term visual light curve parameters of dwarf novae Statistical analysis of the long-term visual light curve parameters of dwarf novae

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...389..478a&link_type=abstract

Astronomy and Astrophysics, v.389, p.478-484 (2002)

Astronomy and Astrophysics

Astrophysics

17

Stars: Dwarf Novae, Stars: Novae, Cataclysmic Variables, Stars: Variables: General

Scientific paper

The long-term visual light curve parameters of 36 dwarf novae are measured. The data is anayzed in search of likely relationships among the light curve parameters and system parameters. New relations of the orbital period with the mean light curve parameters are given. Our findings for the correlation analysis of individual systems agree with some of the results in previous studies. Almost all of the systems in this study have a bimodal frequency distribution of the outburst duration. By comparing the observational correlations with their theoretical counterparts, we find that the value of the viscosity parameter of the disk instability model is alphahot ~0.2.

Affiliated with

Also associated with

No associations

Rating

Statistical analysis of the long-term visual light curve parameters of dwarf novae does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Statistical analysis of the long-term visual light curve parameters of dwarf novae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Statistical analysis of the long-term visual light curve parameters of dwarf novae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-958867