Obtaining normalised component spectra with FDBinary

Details Obtaining normalised component spectra with FDBinary Obtaining normalised component spectra with FDBinary

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..318..111i&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

28

Scientific paper

We discuss the problem of the normalisation of stellar spectra obtained through spectral disentangling of a time series of spectra of a double-lined spectroscopic binary and describe our disentangling code FDBinary. We consider in detail the case of component stars with a time-independent flux ratio. The component spectra are then uniquely determined only up to a constant term. Additionally, due to deviations between the data and the model assumptions, the component spectra may be distorted and present undulations in the continua.

Affiliated with

Also associated with

No associations

Rating

Obtaining normalised component spectra with FDBinary 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 Obtaining normalised component spectra with FDBinary, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Obtaining normalised component spectra with FDBinary will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1020608