Spectroscopic observations of emission-line stars in the Orion. I - ORI OB 1b region

Details Spectroscopic observations of emission-line stars in the Orion. I - ORI OB 1b region Spectroscopic observations of emission-line stars in the Orion. I - ORI OB 1b region

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasj...44...91k&link_type=abstract

PASJ: Publications of the Astronomical Society of Japan (ISSN 0004-6264), vol. 44, no. 2, 1992, p. 91-99.

Astronomy and Astrophysics

Astronomy

11

Emission Spectra, Spectral Energy Distribution, Spectral Line Width, Stellar Spectra, T Tauri Stars, Astronomical Spectroscopy, H Alpha Line, H Beta Line, Hertzsprung-Russell Diagram, Orion Constellation

Scientific paper

The results of spectroscopic observations for 34 emission-line stars (ELSs) detected in the Orion Belt (Ori OB 1b) region are presented. Spectral classification and measurements of the H-alpha and H-beta emission intensities are carried out, and their spectral behaviors are compared with those of classical and weak-emission-line T Tauri stars. It is then found that the observed ELSs are highly probably T Tauri-type stars in most cases.

Affiliated with

Also associated with

No associations

Rating

Spectroscopic observations of emission-line stars in the Orion. I - ORI OB 1b region 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 Spectroscopic observations of emission-line stars in the Orion. I - ORI OB 1b region, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopic observations of emission-line stars in the Orion. I - ORI OB 1b region will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1739525