Hourly variations in O VI P Cygni profiles of hot stars

Details Hourly variations in O VI P Cygni profiles of hot stars Hourly variations in O VI P Cygni profiles of hot stars

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...213l..61y&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 213, Apr. 15, 1977, p. L61-L65.

Astronomy and Astrophysics

Astrophysics

60

Hot Stars, Line Spectra, Periodic Variations, Stellar Spectra, Ultraviolet Absorption, Absorption Spectra, Early Stars, Oao 3, Photomultiplier Tubes, Satellite Observation, Stellar Mass Accretion, Stellar Winds

Scientific paper

Significant changes in the ultraviolet absorption profiles are reported in the spectra of Delta Ori A, Iota Ori, and Zeta Pup. The present data show changes in count rates in excess of 30 per cent at velocities more negative than -900 km/s, if these data are interpreted as being dominated by O VI absorption in stellar winds. The time scales range from 1 to 6 hours.

Affiliated with

Also associated with

No associations

Rating

Hourly variations in O VI P Cygni profiles of hot 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 Hourly variations in O VI P Cygni profiles of hot stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hourly variations in O VI P Cygni profiles of hot stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1616797