The Spectrum analysis of three chromospherically active binary stars.

Details The Spectrum analysis of three chromospherically active binary stars. The Spectrum analysis of three chromospherically active binary stars.

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999pyuno....s.367g&link_type=abstract

Publications of the Yunnan Observatory, Suppl. 1999, p. 367 - 371

Astronomy and Astrophysics

Astronomy

By Draconis Stars: Lithium, By Draconis Stars: Metal Abundances

Scientific paper

The authors present the research results on new CCD spectroscopic observations of three chromospherically active binary stars (BY Dra class), which were obtained by means of Coudé echelle spectrograph fed by the 2.16 m telescope at Beijing Astronomical Observatory. With the aid of stellar model atmosphere, the autors have analyzed these spectra and derived the average metal abundance and Li abundance of three systems. Using two special spectral lines, they have alsop discussed the chromospheric activity indicators of them.

Affiliated with

Also associated with

No associations

Rating

The Spectrum analysis of three chromospherically active binary 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 The Spectrum analysis of three chromospherically active binary stars., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Spectrum analysis of three chromospherically active binary stars. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1587083