TiO band strengths in metal-rich globular clusters IV - The solar neighborhood sequence

Details TiO band strengths in metal-rich globular clusters IV - The solar neighborhood sequence TiO band strengths in metal-rich globular clusters IV - The solar neighborhood sequence

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pasp...94..223m&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 94, Apr. 1982, p. 223-225.

Astronomy and Astrophysics

Astronomy

5

Globular Clusters, Infrared Spectra, Spectral Bands, Stellar Spectrophotometry, Titanium Oxides, Abundance, Giant Stars, Late Stars, M Stars, Near Infrared Radiation, Spectral Line Width, Stellar Atmospheres, Stellar Temperature

Scientific paper

TiO band strengths and near infrared color indices have been measured in
a sample of nearby late-type giants for the purpose of comparison with
observations in metal-rich globular clusters. Transformations to the
Wing narrow-band system are determined.

Affiliated with

Also associated with

No associations

Rating

TiO band strengths in metal-rich globular clusters IV - The solar neighborhood sequence 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 TiO band strengths in metal-rich globular clusters IV - The solar neighborhood sequence, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and TiO band strengths in metal-rich globular clusters IV - The solar neighborhood sequence will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-843429