eta Car emission spectrum (1700-10400Å) (Zethson+, 2012)

Details eta Car emission spectrum (1700-10400Å) (Zethson+, 2012) eta Car emission spectrum (1700-10400Å) (Zethson+, 2012)

Apr 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ycat..35409133z&link_type=abstract

VizieR On-line Data Catalog: J/A+A/540/A133. Originally published in: 2012A&A...540A.133Z

Physics

Stars: Variable, Spectroscopy

Scientific paper

The spectra were recorded in a low state (March 1998) and an early high state (February 1999) with the Hubble Space Telescope/Space Telescope Imaging Spectrograph (HST/STIS) from 1640 to 10400Å using the 52"x0.1" aperture centered on Eta Carinae at position angle, PA=332 degrees. Extractions of the reduced spectrum including both Weigelt B and D, 0.28" in length along the slit, were used to identify the narrow, nebular emission lines, measure their wavelengths and estimate their fluxes.
A linelist of 2500 lines is presented for the high and low states of the combined Weigelt blobs B and D.
(1 data file).

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