CN and CH line strengths in 8 Galactic GlCl (Kayser+, 2008)

Details CN and CH line strengths in 8 Galactic GlCl (Kayser+, 2008) CN and CH line strengths in 8 Galactic GlCl (Kayser+, 2008)

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..34860437k&link_type=abstract

VizieR On-line Data Catalog: J/A+A/486/437. Originally published in: 2008A&A...486..437K

Physics

Clusters: Globular, Abundances

Scientific paper

The spectroscopic data were obtained in May 2002 and July 2004 at the VLT/UT4 at ESO/Paranal (Chile) with the multi-slit spectroscopy instrument FORS2/MXU. FORS2 provides a field of view of 6.8'x6.8'. The observations of M 55 were obtained in 2002. The observations obtained in 2004 were dedicated to CN and CH measurements in seven further Galactic globular clusters (M 15, M 22, M 55, NGC 288, NGC 362, NGC 5286, Palomar 12, and Terzan 7) spanning a large range in metallicity (-2.26<[Fe/H]}<-0.58dex).
(1 data file).

Affiliated with

Also associated with

No associations

Rating

CN and CH line strengths in 8 Galactic GlCl (Kayser+, 2008) 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 CN and CH line strengths in 8 Galactic GlCl (Kayser+, 2008), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CN and CH line strengths in 8 Galactic GlCl (Kayser+, 2008) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1482256