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Astron. Astrophys. 326, 271-276

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Mid infrared spectral observations of UX Orionis*

H.-G. Reimann1, J. Gürtler1, C. Friedemann1, and H. U. Käufl2

1Friedrich-Schiller-Universität Jena, Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergäßchen 2, D-07745 Jena, Germany
2European Southern Observatory, D-85748 Garching, Germany

Received 21 October 1996 / Accepted 25 April 1997


The circumstellar infrared emission of the evolutionarily young irregular variable UX Orionis has been investigated. The observed spectral energy distribution has been modelled by radiative transfer calculations and the parameters for a spherically symmetric envelope have been derived. Two mid-infrared spectra of UX Orionis were obtained with the Thermal Infrared Multimode Instrument (TIMMI) at the ESO 3.6-m telescope. The spectra show the presence of a nearly structureless silicate emission band. Comparison with laboratory data indicates that the circumstellar silicate grains should have radii of FORMULA 0.75-1µm.

Key words: stars: individual: UX Ori - stars: circumstellar matter - (ISM:) dust, extinction - infrared: stars

*Based on observations collected at the European Southern Observatory, La Silla, Chile.

Send offprint requests to: H.-G. Reimann

© European Southern Observatory (ESO) 1997

Online publication: September 9, 1997
Last change: April 20, 1998