A newH α survey of chromospherically active binaries (II)

Details A newH α survey of chromospherically active binaries (II) A newH α survey of chromospherically active binaries (II)

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.246...39x&link_type=abstract

Astrophysics and Space Science, Volume 246, Issue 1, pp.39-50

Astronomy and Astrophysics

Astrophysics

Scientific paper

We have obtained CCD spectra for 30 chromospherically active binaries using the 2.16 m telescope at Beijing Observatory in 1995. Our purpose was to search for the presence ofH α emission which is characteristic of stars with extreme levels of chromospheric activity. Spectra of V711 Tau, V471 Tau, HD 12545 and V833 Tau presentedH α emission above the continuum in the different degree. TheH α behavior of the other observed 26 active binaries, which were unknown in CABS (1993), has been discovered in this paper. TheH α profiles of the most among 26 systems are partially filled-in by chromospheric emission. TheH α profiles of a few systems show a pure absorption line. The results are given in Table I.

Affiliated with

Also associated with

No associations

Rating

A newH α survey of chromospherically active binaries (II) 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 newH α survey of chromospherically active binaries (II), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A newH α survey of chromospherically active binaries (II) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1644019