The circumstellar gas around Beta Pictoris

Details The circumstellar gas around Beta Pictoris The circumstellar gas around Beta Pictoris

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.263..569l&link_type=abstract

In ESA Proceedings of an International Symposium on New Insights in Astrophysics. Eight Years of UV Astronomy with IUE p 569-57

Astronomy and Astrophysics

Astrophysics

1

Accretion Disks, Stellar Envelopes, Stellar Mass Accretion, Iue, Red Shift, Stellar Spectra, Ultraviolet Spectra

Scientific paper

The red shifted components seen in IUE ultraviolet and visual lines of the gaseous component of the disk ground Beta Pictoris are discussed. They may be due to infalling of gas. Changes in time could be explained by strong inhomogeneities within 0.5 AU from the star. However, explanations based on stellar surface and near surface phenomena are feasible.

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