The Beta Pictoris circumstellar disk. IV - Redshifted UV lines

Details The Beta Pictoris circumstellar disk. IV - Redshifted UV lines The Beta Pictoris circumstellar disk. IV - Redshifted UV lines

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...173..289l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 173, no. 2, Feb. 1987, p. 289-292.

Astronomy and Astrophysics

Astrophysics

68

Line Spectra, Red Shift, Stellar Envelopes, Ultraviolet Spectra, Variable Stars, Absorption Spectra, Iron, Iue, Magnesium

Scientific paper

Several new and archive observations with the International Ultraviolet Explorer have confirmed the variability of the UV circumstellar absorption lines of Fe II and Mg II toward β Pic. The authors furthermore show that all these variations take place on the red wing of the lines, in material which is moving toward the star. Tentative scenarios are suggested.

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