The bright pre-main sequence variable HR 5999 - Report of a mini-workshop held in Amsterdam on 7 May, 1984

Details The bright pre-main sequence variable HR 5999 - Report of a mini-workshop held in Amsterdam on 7 May, 1984 The bright pre-main sequence variable HR 5999 - Report of a mini-workshop held in Amsterdam on 7 May, 1984

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985iraj...17...79t&link_type=abstract

Irish Astronomical Journal (ISSN 0021-1052), vol. 17, Sept. 1985, p. 79-97.

Mathematics

Dynamical Systems

13

Atmospheric Models, Brightness Distribution, Pre-Main Sequence Stars, Stellar Atmospheres, Stellar Spectra, Variable Stars, Astronomical Photometry, Astronomical Spectroscopy, Dynamical Systems, Iue, Light Curve, Stellar Oscillations, X Ray Astronomy

Scientific paper

A meeting to review the reduced coordinated observations by EXOSAT, IUE and ground-based instruments of the bright and variable Herbig A7e star HR 5999 is summarized. The attempt was to delineate the relationship between the various observable quantities of its atmosphere (colors, emission-line fluxes, wind velocities, etc.) in order to develop a dynamical model of the extended atmosphere. The observations were made around September 11, 1983.

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