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Azimuthal structures in the wind and chromosphere of the herbig Ae star ab aur. preliminary results from the MUSICOS 1992 campaign
Authors:C. Catala  T. Böhm  J. -F. Donati  T. Simon  A. Welty  E. Houdebine  L. Huang  S. Jiang  D. Zhai  J. Neff  B. H. Foing  K. Ghosh  J. Butler  A. Collier-Cameron  J. Baudrand  J. Czarny  B. Carter  D. Rees  M. Semel  G. Cutispoto  M. Rodonò
Affiliation:(1) Département de Recherche Spatiale et Unité de Recherche associée au CNRS 264, Observatoire de Paris, Section de Meudon, France;(2) Département d'Astrophysique Extragalactique et de Cosmologie et Unité de Recherche associée au CNRS 173, Observatoire de Paris, Section de Meudon, France;(3) University of Hawaii, USA;(4) Pennsylvania State University, USA;(5) Armagh Observatory, U.K.;(6) Beijing Astronomical Observatory, China;(7) Solar System Division, ESA Space Science Department, ESTEC SO, The Netherland;(8) Vainu Bappu Observatory, India;(9) University of Sussex, U.K.;(10) University of New South Wales, Australia;(11) CSIRO, Australia;(12) Observatoire de Paris-Meudon, France;(13) Catania Observatory, Italy
Abstract:MUSICOS (for MUlti-SIte COntinuous Spectroscopy) is an international project to facilitate and organize world-wide multi-site campaigns in high resolution spectroscopy, in view of obtaining a complete time coverage of various types of variable stellar phenomena.In the framework of this project a vast spectroscopic campaign was organized in December 1992, involving 8 sites well distributed in longitude around the Earth. The observations concerned three scientific programs, among which was the study of azimuthal structures in the wind and chromosphere of the pre-Main-Sequence Herbig Ae star AB Aur.The Hei 5876 angst line of AB Aur, which is formed in the expanding chromosphere of this star, in the innermost parts of its wind, was monitored at a resolution of 30000, nearly continuously for about 4 days. A spectacular variability of this line was discovered, the profile changing from pure emission to a composite profile including a deep absorption component in the course of a few hours. This variability can be the signature of azimuthal structures in the wind of AB Aur.We present the data collected during the campaign, and discuss possible interpretations of the spectacular variations of the Hei 5876 angst line.ESA/VILSPAUniversity of British Columbia CanadaBased on observations obtained during the MUSICOS 92 MUlti-SIte COntinuous Spectroscopic campaign from the National Solar Observatory McMath/Pierce 1.5 m, University of Hawaii 2.2 m, Beijing Observatory Xinglong 2.16 m, La Palma 4.2 m William Herschel Telescope, and Observatoire de Haute-Provence 1.52 m telescopes.Presented at the lsquoCosmic Winds and the Heliospherersquo Conference in Tucson, Arizona, U.S.A., October 18–22, 1993.Visiting Astronomer, Kitt Peak National Observatory, National Optical Astronomy Observatories, which is operated by the Association of Universities for Research in Astronomy, Inc., under cooperative agreement with the National Science Foundation.Visiting Astronomer National Solar Observatory, National Optical Astronomy Observatories, which is operated by the Association of Universities for Research in Astronomy, Inc., under cooperative agreement with the National Science Foundation.
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