Abundance analysis of LSS 3378 (Pandey+, 2006)

Details Abundance analysis of LSS 3378 (Pandey+, 2006) Abundance analysis of LSS 3378 (Pandey+, 2006)

Feb 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..73691677p&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/369/1677. Originally published in: 2006MNRAS.369.1677P

Physics

Stars: Variable, Abundances: Peculiar

Scientific paper

The spectrum of LSS 3378 was obtained on 2002 June 19 with the 4-m Blanco telescope and the Cassegrain echelle spectrograph at Cerro Tololo Inter-American Observatory (CTIO) in Chile. Three exposures of 25-min each, spectra covering the wavelength interval 50008200{AA} without gaps, were recorded at a resolving power of R=30000. The Image Reduction and Analysis Facility (IRAF) software packages were used to reduce the recorded spectra.
(1 data file).

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