Abundance of nine beta Cephei stars (Morel+, 2006)

Details Abundance of nine beta Cephei stars (Morel+, 2006) Abundance of nine beta Cephei stars (Morel+, 2006)

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycat..34570651m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/457/651. Originally published in: 2006A&A...457..651M

Computer Science

Stars: Early-Type, Abundances

Scientific paper

The equivalent widths (EWs) were measured on high-resolution spectra obtained with various echelle spectrographs (see Table 2 of paper for further details). Our EWs are systematically larger than the values quoted by Gies & Lambert (1992ApJ...387..673G) for the seven stars in common, but a similar trend is evident when comparing their values with previous measurements in the literature (see their Fig.4). This is likely to result from their use of Gaussian fitting instead of the direct integration used in our case. The same conclusion holds for the EWs of xi1 CMa presented by Hambly et al. (1996MNRAS.278..811H).
(1 data file).

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