The Abundance Ratio C/O in the Atmospheres of 89 Carbon Stars

Details The Abundance Ratio C/O in the Atmospheres of 89 Carbon Stars The Abundance Ratio C/O in the Atmospheres of 89 Carbon Stars

Apr 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ap%26ss.249..235e&link_type=abstract

Astrophysics and Space Science, Volume 249, Issue 2, pp.235-256

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

The abundance ratio C/O in the atmospheres of 89 faint carbon stars are detected on the basis of spectra obtained on 2.6 m telescope of Byurakan AO. The frequency distribution of C/O in the Perseus galactic arm differs from that in the Orion arm. The conclusion is made that the reason of the difference may be the heavy element abundance differences in these galactic arms.

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