Chemical Composition of the RS CVn-TYPE Star Lambda Andromedae

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

Photospheric parameters and chemical composition are determined for the single-lined chromospherically active RS CVn-type star {\lambda} And (HD 222107). From the high resolution spectra obtained on the Nordic Optical Telescope, abundances of 22 chemical elements and isotopes, including such key elements as 12C, 13C, N and O, were investigated. The differential line analysis with the MARCS model atmospheres gives T eff=4830 K, log g=2.8, [Fe/H]=-0.53, [C/Fe]=0.09, [N/Fe]=0.35, [O/Fe]=0.45, C/N=2.21, 12C/13C = 14. The value of 12C/13C ratio for a star of the RS CVn-type is determined for the first time, and its low value gives a hint that extra-mixing processes may start acting in low-mass chromospherically active stars below the bump of the luminosity function of red giants.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Chemical Composition of the RS CVn-TYPE Star Lambda Andromedae 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 Chemical Composition of the RS CVn-TYPE Star Lambda Andromedae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chemical Composition of the RS CVn-TYPE Star Lambda Andromedae will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-473897

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.