Curve-of-growth analysis of another red giant in M67

Details Curve-of-growth analysis of another red giant in M67 Curve-of-growth analysis of another red giant in M67

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.187..277g&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 187, Apr. 1979, p. 277-281. Research supported by the Science Research

Astronomy and Astrophysics

Astronomy

12

Abundance, Data Reduction, Red Giant Stars, Star Clusters, Stellar Spectrophotometry, Image Tubes, Metallic Stars, Stellar Luminosity, Tables (Data), Wavelengths

Scientific paper

The paper is concerned with the image-tube spectogram of the second-brightest, second-reddest known member of the galactic cluster M67, designated by T626. A curve-of-growth analysis shows that element abundances in T626 are similar to those found in IV-202 within the error limits set by the quality of the data. It is concluded that stars in M67 are not 'super-metal-rich' but may have mild metal deficiencies relative to the sun.

Affiliated with

Also associated with

No associations

Rating

Curve-of-growth analysis of another red giant in M67 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 Curve-of-growth analysis of another red giant in M67, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Curve-of-growth analysis of another red giant in M67 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1436470