New Observations Of The Eclipsing Red Dwarfs In LP133-373

Details New Observations Of The Eclipsing Red Dwarfs In LP133-373 New Observations Of The Eclipsing Red Dwarfs In LP133-373

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21915329v&link_type=abstract

American Astronomical Society, AAS Meeting #219, #153.29

Astronomy and Astrophysics

Astronomy

Scientific paper

We have spectroscopically and photometrically observed the low mass eclipsing binary LP133-373 over several years. The new radial velocities have helped refine the physical characteristics of this important system, particularly the mass ratio, which is close to unity. Velocity curves based on measurements of the H alpha emission lines appear to have a larger amplitude than curves made with absorption line measurements, possibly due to the location of active regions. Additional eclipse timings indicate that the orbital period may be changing and the systemic velocity appears to be changing as well.

Affiliated with

Also associated with

No associations

Rating

New Observations Of The Eclipsing Red Dwarfs In LP133-373 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 New Observations Of The Eclipsing Red Dwarfs In LP133-373, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New Observations Of The Eclipsing Red Dwarfs In LP133-373 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1576797