Energy distribution of main-sequence B stars (Knyazeva+, 1996)

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Stars: Ob, Energy Distributions

Scientific paper

The normal spectral energy distribution in the spectra of main-sequence B stars of five subclasses is presented. Spectral classification and UBV photometry from the fourth edition of the BSC and spectrophotometry from three extensive spectrophotometric catalogs are used. The method of selecting unreddened stars is outlined. The good agreement between the mean color indices in the UBV system calculated for a sample of stars with spectrophotometry and for considerably larger samples of unreddened stars of the corresponding subclasses from the BSC confirms the reliability of the results obtained.
(1 data file).

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Energy distribution of main-sequence B stars (Knyazeva+, 1996) 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 Energy distribution of main-sequence B stars (Knyazeva+, 1996), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Energy distribution of main-sequence B stars (Knyazeva+, 1996) will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-962948

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.