A carbon rich star BD +75deg 348: a binary?

Details A carbon rich star BD +75deg 348: a binary? A carbon rich star BD +75deg 348: a binary?

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...358.1022z&link_type=abstract

Astronomy and Astrophysics, v.358, p.1022-1026 (2000)

Astronomy and Astrophysics

Astrophysics

8

Stars: Evolution, Stars: Abundances, Stars: Chemically Peculiar, Stars: Individual: Bd +75O348

Scientific paper

An LTE abundance analysis of the ``CH-like" star BD +75deg 348, with an unknown evolutionary status, is presented based on high resolution, high signal-to-noise spectra. With [C/Fe] = +0.5 dex and a mean s-process overabundance of [s/Fe] =~ +1.6 dex the peculiar atmospheric composition of BD +75deg 348 is confirmed. The modest iron deficiency, [Fe/H] = -0.8, and the kinematic data support the idea that BD +75deg 348 is an old disk population object. Possible evolutionary stages, that can explain its atmospheric parameters and peculiar chemical composition, are discussed.

Affiliated with

Also associated with

No associations

Rating

A carbon rich star BD +75deg 348: a binary? 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 A carbon rich star BD +75deg 348: a binary?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A carbon rich star BD +75deg 348: a binary? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1387222