Calibrating Stellar Evolution Models and Defining the Radius-Activity and -Metallicity Relations for M dwarfs

Details Calibrating Stellar Evolution Models and Defining the Radius-Activity and -Metallicity Relations for M dwarfs Calibrating Stellar Evolution Models and Defining the Radius-Activity and -Metallicity Relations for M dwarfs

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010noao.prop..111h&link_type=abstract

NOAO Proposal ID #2010A-0111

Physics

Scientific paper

Our goal is to empirically determine the mass-radius relationship of M dwarfs using a sample of F/G/K+M dwarf eclipsing binaries (EBs) in order to establish in detail how the measured radii depend on activity and metallicity. In addition, we aim to make precise measurements of the temperatures and metallicities of known benchmark EBs which lack this information. This will allow for critical testing of theoretical stellar evolution models.

Affiliated with

Also associated with

No associations

Rating

Calibrating Stellar Evolution Models and Defining the Radius-Activity and -Metallicity Relations for M dwarfs 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 Calibrating Stellar Evolution Models and Defining the Radius-Activity and -Metallicity Relations for M dwarfs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Calibrating Stellar Evolution Models and Defining the Radius-Activity and -Metallicity Relations for M dwarfs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1106078