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B[e] Stars pp 137–139Cite as

Analysis of the Emission Line Spectrum of V380 Ori and HD45677

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 233))

Abstract

The ionized metal emission lines in the Herbig Ae/Be star V380 Ori and in the B[e] star HD45677 (FS CMa) have been analysed with the SAC method. We found that probably all the emission lines are optically thick. The analysis of V380 Ori indicates that the principal components of the Fe II emission lines are very probably formed in a rotating disk.

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Author information

Authors and Affiliations

  1. Observatoire de Marseille, 2 Place Le Verrier, F-13248, Marseille Cedex 04, France

    G. Muratorio

  2. Istituto Astronomico dell’Università ”La Sapienza”, Via G.M. Lancisi 29, I-00161, Roma, Italy

    C. Rossi

  3. Institut d’Astrophysique (CNRS), 98 bis Boulevard Arago, F-75014, Paris, France

    M. Friedjung

  4. Istituto di Astrofisica Spaziale (CNR), Via E. Fermi 21, I-00044, Frascati RM, Italy

    R. Viotti

Authors
  1. G. Muratorio
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  2. C. Rossi
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  3. M. Friedjung
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  4. R. Viotti
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Editor information

Editors and Affiliations

  1. Observatoire de Paris-Meudon, France

    Anne Marie Hubert

  2. Observatoire de Strasbourg, France

    Carlos Jaschek

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© 1998 Springer Science+Business Media Dordrecht

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Muratorio, G., Rossi, C., Friedjung, M., Viotti, R. (1998). Analysis of the Emission Line Spectrum of V380 Ori and HD45677. In: Hubert, A.M., Jaschek, C. (eds) B[e] Stars. Astrophysics and Space Science Library, vol 233. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-9014-3_16

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  • DOI: https://doi.org/10.1007/978-94-015-9014-3_16

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-5080-9

  • Online ISBN: 978-94-015-9014-3

  • eBook Packages: Springer Book Archive

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