Heavy element abundances in HD 209621 (Goswami+, 2010)

Details Heavy element abundances in HD 209621 (Goswami+, 2010) Heavy element abundances in HD 209621 (Goswami+, 2010)

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..74040253g&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/404/253. Originally published in: 2010MNRAS.404..253G

Physics

Stars: Carbon, Spectroscopy, Equivalent Widths

Scientific paper

High-resolution spectroscopic observations of HD 209621 were carried out with the High Dispersion Spectrograph (HDS) of the 8.2-m Subaru Telescope on 2005 July 20 at a resolving power of R~50000. The object spectrum was taken with a 5-min exposure. The observed bandpass ran from about 4020 to 6775Å, with a gap of about 75Å, from 5335 to 5410Å, due to the physical spacing of the CCD detectors. Observations of a Th-Ar hollow cathode lamp provided the wavelength calibration.
(1 data file).

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