Nearby B-type stars abundances (Morel+, 2008)

Details Nearby B-type stars abundances (Morel+, 2008) Nearby B-type stars abundances (Morel+, 2008)

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..34870307m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/487/307. Originally published in: 2008A&A...487..307M

Physics

Stars: Nearby, Stars: Early-Type, Stars: B-Type, Abundances

Scientific paper

This Table gives the adopted loggf values, EW measurements (in mA) and line-by-line abundances (on the scale in which log[epsilon(H)]=12). A blank indicates that the EW was not reliably measurable, the line was considered blended for the relevant temperature range or yielded a discrepant abundance. The accuracy of the EW measurements is discussed in Sect.3 of the paper. The wing of HeI 4387.9 was taken as pseudo continuum in the case of NeII 4391.99.
(2 data files).

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