EWs of 31 giant stars of 10 open clusters (Smiljanic+, 2009)

Details EWs of 31 giant stars of 10 open clusters (Smiljanic+, 2009) EWs of 31 giant stars of 10 open clusters (Smiljanic+, 2009)

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..35020267s&link_type=abstract

VizieR On-line Data Catalog: J/A+A/502/267. Originally published in: 2009A&A...502..267S

Physics

Clusters: Open, Stars: Giant, Equivalent Widths

Scientific paper

Equivalent widths (EWs) of a sample of 31 giant stars of 10 open clusters. The list includes lines of NaI, MgI, SiI, CaI, ScII, TiI, VI, VII, CrI, CrII, FeI, FeII, CoI, NiI, YII, CeII, and EuII. For most of the lines, EWs were measured using PeakFit. For some Fe II lines, EWs were measured by fitting Gaussian profiles to the lines with the IRAF task SPLOT. The adopted oscillator strengths (loggfs) and excitation potentials (EP) are also listed. For the stars of the clusters NGC 2360 and NGC 2447 only the FeII EWs are given. The EWs of the remaining lines can be found in Hamdani et al. (2000, Cat. J/A+A/360/509).
(2 data files).

Affiliated with

Also associated with

No associations

Rating

EWs of 31 giant stars of 10 open clusters (Smiljanic+, 2009) 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 EWs of 31 giant stars of 10 open clusters (Smiljanic+, 2009), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and EWs of 31 giant stars of 10 open clusters (Smiljanic+, 2009) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1114247