Volume 496, Number 3, March IV 2009
|Page(s)||759 - 763|
|Section||Stellar structure and evolution|
|Published online||09 February 2009|
The symbiotic star CH Cygni
The broad Lyα emission line explained by shocks
Dipartimento di Astronomia, University of Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy e-mail: [rodolfo.angeloni;piero.rafanelli]@unipd.it
2 School of Physics and Astronomy, Tel-Aviv University, 69978 Tel-Aviv, Israel e-mail: firstname.lastname@example.org
Accepted: 1 April 2008
Context. In 1985, at the end of the active phase 1977-1986, a broad (4000 ) Lyα line appeared in the symbiotic system CH Cygni that had never been observed previously.
Aims. In this work we investigate the origin of this anomalous broad Lyα line.
Methods. We suggest a new interpretation of the broad Lyα based on the theory of charge transfer reactions between ambient hydrogen atoms and post-shock protons at a strong shock front.
Results. We have found that the broad Lyα line originated from the blast wave created by the outburst, while the contemporary optical and UV lines arose from the nebula downstream of the expanding shock in the colliding-wind scenario.
Key words: stars: binaries: symbiotic / stars: individual: CH Cyg
© ESO, 2009
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