Lithium abundances among solar-type pre-main-sequence stars

Details Lithium abundances among solar-type pre-main-sequence stars Lithium abundances among solar-type pre-main-sequence stars

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aj.....98.1444s&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 98, Oct. 1989, p. 1444-1450. Research supported by NSF and NASA.

Astronomy and Astrophysics

Astronomy

73

Abundance, Lithium, Metallicity, Pre-Main Sequence Stars, Spectral Line Width, Stellar Composition, Astronomical Catalogs, Data Sampling, H Alpha Line, Hertzsprung-Russell Diagram

Scientific paper

Measurements of Li I 6707 A line strengths were carried out for two samples of pre-main-sequence (PMS) stars (L 1641 and Taurus-Auriga), and the Li abundances estimated for PMS stars are compared with those deduced from observations of Li line strengths for main-sequence stars in the Alpha Persei cluster. It was found that the maximum Li abundances among the PMS stars with solar mass values greater than 1.0 exceed the maximum abundances for Alpha Per stars by at least 0.3 dex. Some PMS stars, including few apparently young stars, showed large (greater than 1.0 dex) Li depletion, and some apparently old PMS stars showed little or no depletion.

Affiliated with

Also associated with

No associations

Rating

Lithium abundances among solar-type pre-main-sequence stars 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 Lithium abundances among solar-type pre-main-sequence stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Lithium abundances among solar-type pre-main-sequence stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1527531