The Metal Abundances of NGC 188 and NGC 6791 from Low-Resolution Spectra

Details The Metal Abundances of NGC 188 and NGC 6791 from Low-Resolution Spectra The Metal Abundances of NGC 188 and NGC 6791 from Low-Resolution Spectra

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003pasp..115...96w&link_type=abstract

The Publications of the Astronomical Society of the Pacific, Volume 115, Issue 803, pp. 96-103.

Astronomy and Astrophysics

Astronomy

23

Stars: Abundances, Galaxy: Open Clusters And Associations: Individual: Ngc Number: Ngc 6791, Galaxy: Open Clusters And Associations: Individual: Ngc Number: Ngc 188

Scientific paper

Analysis of low-resolution spectra of K giants in the old open clusters NGC 188 and NGC 6791 yields [Fe/H]=0.075+/-0.045+/-σsys for NGC 188 and [Fe/H]=0.320+/-0.023+/-σsys for NGC 6791. The term σsys represents the drift between our underlying star catalog's abundance scale and the true abundance scale. Star R23 in NGC 6791 has [Fe/H]>0.6 according to our analysis and deserves further study.

Affiliated with

Also associated with

No associations

Rating

The Metal Abundances of NGC 188 and NGC 6791 from Low-Resolution Spectra 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 The Metal Abundances of NGC 188 and NGC 6791 from Low-Resolution Spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Metal Abundances of NGC 188 and NGC 6791 from Low-Resolution Spectra will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1321219