Photometric and Spectroscopic Mass Ratios of W-Ursae Stars

Details Photometric and Spectroscopic Mass Ratios of W-Ursae Stars Photometric and Spectroscopic Mass Ratios of W-Ursae Stars

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983msngr..33...31m&link_type=abstract

The Messenger, No.33, P.31, 1983

Astronomy and Astrophysics

Astrophysics

Scientific paper

W UMa binary stars represent a typieal case of astronomieal objects for which theory and teehniques of data reduetion are much more developed and up to date than observations. While the analysis of photometrie observations by means of synthetic light curve methods (Wilson and Oevinney, 1971 Astrophysical JOurnal, 166, 605) yields good photometrie elements, the absence of reliable spectroscopie data makes the determination 0f the absolute elements 0f these systems and therefore of their evolutionary status problematic.

Affiliated with

Also associated with

No associations

Rating

Photometric and Spectroscopic Mass Ratios of W-Ursae Stars 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 Photometric and Spectroscopic Mass Ratios of W-Ursae Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photometric and Spectroscopic Mass Ratios of W-Ursae Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1593430