pith. machine review for the scientific record. sign in

arxiv: astro-ph/9712093 · v2 · submitted 1997-12-05 · 🌌 astro-ph

ORFEUS-SPAS II EUV Spectroscopy of epsilon Canis Majoris (B2 II)

classification 🌌 astro-ph
keywords canisepsilonextreme-ultravioletlambdamajorisorfeus-spasareaassess
0
0 comments X
read the original abstract

We report on extreme-ultraviolet (EUV) spectroscopic observations of the B bright giant epsilon Canis Majoris made during the ORFEUS-SPAS II mission. We assess the performance of the instrument in the EUV and find that the effective area is roughly 3 times that of the Extreme-Ultraviolet Explorer (EUVE) long-wavelength spectrometer and that the spectral resolution is lambda/Delta(lambda) = 1250. We identify most of the features, qualitatively compare different models, and examine the wind-broadened O V and Si IV lines, which display blue edge velocities up to 800 km/s.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.