Magnetic activity and orbital dynamics of the K-dwarf triple system DH Leonis

Details Magnetic activity and orbital dynamics of the K-dwarf triple system DH Leonis Magnetic activity and orbital dynamics of the K-dwarf triple system DH Leonis

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..318..251i&link_type=abstract

In Spectroscopically and Spatially Resolving the Components of the Close Binary Stars, Proceedings of the Workshop held 20-24 Oc

Astronomy and Astrophysics

Astronomy

Scientific paper

DH Leo, a (K0V+K7V)/K5V type spectroscopic triple system consisting of an active close binary (Porb˜ 1.07 d) and a distant, slowly rotating tertiary has been observed spectroscopically in 2000 and 2002. The orbit of the tertiary has been estimated using long-term cross-correlation radial velocities and results from astrometric studies. Chromospheric activity patterns of the close binary components has been resolved using semi-empirically synthesized Hα spectra. Following a simple but statistically convenient method, the slowly-rotating tertiary has been found to be inactive within the errors of measurement.

Affiliated with

Also associated with

No associations

Rating

Magnetic activity and orbital dynamics of the K-dwarf triple system DH Leonis 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 Magnetic activity and orbital dynamics of the K-dwarf triple system DH Leonis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetic activity and orbital dynamics of the K-dwarf triple system DH Leonis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1020653