Scanner Observations of the Be-Stars Nu-Geminorum Kappa-Orionis Beta-Monocerotis Omega-Canis

Details Scanner Observations of the Be-Stars Nu-Geminorum Kappa-Orionis Beta-Monocerotis Omega-Canis Scanner Observations of the Be-Stars Nu-Geminorum Kappa-Orionis Beta-Monocerotis Omega-Canis

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..78..419g&link_type=abstract

Astrophysics and Space Science, Volume 78, Issue 2, pp.419-425

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

The photoelectric spectrophotometric scans of the Be stars ν Gem, κ Ori, β Mon and ω CMa have been analyzed to find out few stellar parameters. The absolute energy distributions of these stars in the wavelength range λλ 350 750 nm have been given. Their effective temperatures and gravities have been estimated from comparisons with non-LTE model atmospheres. The stars ν Gem and β Mon have been found to have Balmer discontinuities in emission. The excess emission in the region λλ 620 750 nm has been observed for β Mon and ω CMa. The evolutionary aspects of these stars are discussed and their masses have been estimated.

Affiliated with

Also associated with

No associations

Rating

Scanner Observations of the Be-Stars Nu-Geminorum Kappa-Orionis Beta-Monocerotis Omega-Canis 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 Scanner Observations of the Be-Stars Nu-Geminorum Kappa-Orionis Beta-Monocerotis Omega-Canis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Scanner Observations of the Be-Stars Nu-Geminorum Kappa-Orionis Beta-Monocerotis Omega-Canis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1744274