A spectrophotometric study of the Be star HD 184279

Details A spectrophotometric study of the Be star HD 184279 A spectrophotometric study of the Be star HD 184279

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....41..199s&link_type=abstract

Astronomy and Astrophysics, vol. 41, no. 2, June 1975, p. 199-202.

Astronomy and Astrophysics

Astrophysics

3

Absorption Spectra, B Stars, H Alpha Line, Spectral Line Width, Stellar Spectrophotometry, Helium, Luminous Intensity, Stellar Atmospheres, Stellar Envelopes

Scientific paper

Spectra of the Be star HD 184279 have been studied. The H-alpha line
appears in emission, and its profile is given. The equivalent widths and
the intensities of the measured absorption lines are also given. The
lines observed in HD 184279 are used to estimate the central star's
atmospheric parameters as well as those of its surrounding shell.

Affiliated with

Also associated with

No associations

Rating

A spectrophotometric study of the Be star HD 184279 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 A spectrophotometric study of the Be star HD 184279, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A spectrophotometric study of the Be star HD 184279 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-747969