Physical parameters of a sample of M dwarfs from high-resolution near-infrared spectra

Details Physical parameters of a sample of M dwarfs from high-resolution near-infrared spectra Physical parameters of a sample of M dwarfs from high-resolution near-infrared spectra

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epjwc..1604006d&link_type=abstract

Research, Science and Technology of Brown Dwarfs and Exoplanets: Proceedings of an International Conference held in Shangai on O

Computer Science

Scientific paper

We show preliminary results about the effective temperature, surface gravity, and projected rotational velocity of eleven M dwarfs from the comparison of high-resolution near-infrared spectra with resolving power of ~20,000 and atmosphere synthetic models. Our results are in good agreement with those found in the literature. We find that the haze of observed absorption features (mostly water vapor) is relatively well modeled by the synthetic spectra.

Affiliated with

Also associated with

No associations

Rating

Physical parameters of a sample of M dwarfs from high-resolution near-infrared spectra 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 Physical parameters of a sample of M dwarfs from high-resolution near-infrared spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Physical parameters of a sample of M dwarfs from high-resolution near-infrared spectra will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-992103