Column densities of interstellar gas in the direction of the star epsilon ORI (B0 IA)

Details Column densities of interstellar gas in the direction of the star epsilon ORI (B0 IA) Column densities of interstellar gas in the direction of the star epsilon ORI (B0 IA)

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.220..279m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 220, no. 2, p. 279-287

Astronomy and Astrophysics

Astrophysics

Abundance, Aluminum, Gas Density, Interstellar Gas, Iron, Line Spectra, Nickel, Silicon, Sulfur, Ultraviolet Absorption, Zinc, Iue, Oao 3, Orion Constellation

Scientific paper

We have investigated the star epsilon Ori with International Ultraviolet
Explorer (IUE) high resolution SWP spectrum in order to derive curve of
growth and column densities of Al II, Si II, S II, Fe II, Ni II and Zn
II. It has been possible to fit these ions on one empirical curve of
growth with a velocity parameter b = 11 km/sec for the star studied.

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