Emission lines in optical spectrum of 3 Cen A (Wahlgren+, 2004)

Details Emission lines in optical spectrum of 3 Cen A (Wahlgren+, 2004) Emission lines in optical spectrum of 3 Cen A (Wahlgren+, 2004)

Feb 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ycat..34181073w&link_type=abstract

VizieR On-line Data Catalog: J/A+A/418/1073. Originally published in: 2004A&A...418.1073W

Physics

Abundances, Equivalent Widths, Spectroscopy, Stars: Peculiar

Scientific paper

Weak emission lines in the optical spectrum of the helium-weak chemically peculiar star 3 Cen A are tabulated. The observed wavelengths, line identification information and equivalent widths are presented based on data obtained with the ESO 1.5m telescope and FEROS instrument (16-17 May 2000) and the VLT with UVES spectrograph (24 June 2001).
Table 2 is a listing of all recorded emission lines arranged by wavelength and including unidentified features. Table 3 arranges the identified lines according to their ion and multiplet.
(2 data files).

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