Separating the components of close binary stars

Details Separating the components of close binary stars Separating the components of close binary stars

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..318..433g&link_type=abstract

In Spectroscopically and Spatially Resolving the Components of the Close Binary Stars, Proceedings of the Workshop held 20-24 Oc

Astronomy and Astrophysics

Astronomy

1

Scientific paper

At this remarkable meeting astronomers gathered to compare methods and results on the separation of the flux from the components of binary stars. Here I will present a brief review of some of the new techniques that will soon become the commonplace working tools in this field. I will also highlight some of the exciting new observational results that were presented. We are entering an era where important results will come from a combination of observational methods (astrometry, high angular resolution measurements, photometry, spectroscopy, and multiwavelength studies). These techniques will allow us to push investigations into regions of binary separation and flux ratio that are unexplored realms at the moment.

Affiliated with

Also associated with

No associations

Rating

Separating the components of close binary 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 Separating the components of close binary stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Separating the components of close binary stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1020809