High-resolution spectral analysis of the mildly metal-poor stars II. Chemical abundances

Details High-resolution spectral analysis of the mildly metal-poor stars II. Chemical abundances High-resolution spectral analysis of the mildly metal-poor stars II. Chemical abundances

Aug 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002acasn..43..257q&link_type=abstract

Acta Astronomica Sinica, vol.43, no.3, p. 257-263

Astronomy and Astrophysics

Astronomy

Stars: Abundances, Stars: Atmospheres, Stars: Individual: Hd22484, Hd51530, Hd59984

Scientific paper

Based on the first paper, here the model parameters of a set of sample stars and the chemical abundances for nine elements are presented. The relations between the elemental abundances and [Fe/H] are also discussed. On average, [Na/Fe] tends to -0.01dex and shows solar pattern. The ? elements, Si and Ca, show the same abundance patterns, while [Ti/Fe] has a large scatter. The abundances of these three elements all decrease with [Fe/H] increasing. The iron-peak elements V, Cr, Ni show a large scatter at different metallicity, and [Ca/Fe] is overabundant in all the sample stars, while [Mn/Fe] is definitely under-abundant and increases with the metallicity increasing.

Affiliated with

Also associated with

No associations

Rating

High-resolution spectral analysis of the mildly metal-poor stars II. Chemical abundances 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 High-resolution spectral analysis of the mildly metal-poor stars II. Chemical abundances, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High-resolution spectral analysis of the mildly metal-poor stars II. Chemical abundances will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1673580