VLT-FLAMES survey of massive stars (Hunter+, 2007)

Details VLT-FLAMES survey of massive stars (Hunter+, 2007) VLT-FLAMES survey of massive stars (Hunter+, 2007)

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..34660277h&link_type=abstract

VizieR On-line Data Catalog: J/A+A/466/277. Originally published in: 2007A&A...466..277H

Physics

Equivalent Widths, Stars: B-Type, Abundances

Scientific paper

Files table3.dat, table4.dat and table5.dat contain the equivalent widths and abundances estimates of the observed metal lines for B-type stars in NGC 6611, N11 and NGC 346 respectively. The equivalent widths of the spectral lines have been measured using the line fitting program ELF in the spectral analysis package DIPSO (Howarth et al., 1994, Starlink User Note, No. 50.15). The nitrogen equivalent widths and abundances are upper limits for objects N11-037, N11-047, N11-101, NGC 346-029, NGC 346-039, NGC 346-040, NGC 346-043, NGC 346-044 and NGC 346-075.
table6.dat contains details of the adopted atomic data for the absorption lines considered in this analysis. Model atoms are discussed in Lanz & Hubeny (2003ApJS..146..417L) and Allende Prieto et al. (2003ApJS..147..363A), see Dufton et al. (2005, Cat. ) for further details. Note, the loggf values of the Si II lines at 4128 and 4131 angstroms have been updated to include improved atomic data (A. Korn, private communication).
(5 data files).

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