Hα emission from pre-main sequence stars.

Details Hα emission from pre-main sequence stars. Hα emission from pre-main sequence stars.

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26as..114..439f&link_type=abstract

Astronomy and Astrophysics Supplement, v.114, p.439

Astronomy and Astrophysics

Astrophysics

62

Stars: Formation, Stars: Pre-Main Sequence, Line: Profiles

Scientific paper

We present the results of an Hα emission line observational study of a sample of 75 pre-main sequence stars consisting of 17 HAEBE, 47 CTT and 11 WTT stars. Approximately half of the stars are faint, with a brightness in the V band >13. The spectra have been taken at resolutions =~30km/s and =~80km/s. The data shown provide information on equivalent width, radial velocity, variability and line profile.

Affiliated with

Also associated with

No associations

Rating

Hα emission from pre-main sequence 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 Hα emission from pre-main sequence stars., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hα emission from pre-main sequence stars. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1252616