Equivalent widths for giants in metal rich globular clusters. I

Details Equivalent widths for giants in metal rich globular clusters. I Equivalent widths for giants in metal rich globular clusters. I

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26as...68...21g&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 68, no. 1, Feb. 1987, p. 21-31.

Astronomy and Astrophysics

Astrophysics

10

Giant Stars, Globular Clusters, Late Stars, Metallicity, Stellar Spectra, Abundance, Spectral Line Width, Stellar Atmospheres

Scientific paper

Observations of giants in five metal rich globular clusters, obtained in October 1984 and June 1985 using the CASPEC spectrograph of the 3.6-m ESO telescope at La Silla, are presented, and equivalent widths for about 100 lines in each spectra were obtained using a line integration code. S/N ratios ranged from about 50 for the fainter globular cluster stars to greater than 100 for the Alpha Boo spectra. Equivalent widths measured in the Alpha Boo spectra were found to be generally larger by about 20 mA than those obtained by Maeckle et al. (1975), due to the lower resolution of the present spectra.

Affiliated with

Also associated with

No associations

Rating

Equivalent widths for giants in metal rich globular clusters. I 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 Equivalent widths for giants in metal rich globular clusters. I, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Equivalent widths for giants in metal rich globular clusters. I will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1010851