2009
DOI: 10.1111/j.1365-2966.2009.14792.x
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Shock fronts in the symbiotic system BI Crucis

Abstract: We investigate the symbiotic star BI Crucis (BI Cru) through a comprehensive and self-consistent analysis of the spectra emitted in three different epochs: 1960s, 1970s and late 1980s. In particular, we would like to find out the physical conditions in the shocked nebula and in the dust shells, as well as their location within the symbiotic system, by exploiting both photometric and spectroscopic data from radio to UV. We suggest a model which, on the basis of optical imaging, emission-line ratios and spectral… Show more

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Cited by 11 publications
(19 citation statements)
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“…BI Cru. A careful analysis of BI Cru as a colliding‐wind SS has been recently described by Contini et al (2009b). We refer to that paper for any further details about models and results.…”
Section: Resultsmentioning
confidence: 99%
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“…BI Cru. A careful analysis of BI Cru as a colliding‐wind SS has been recently described by Contini et al (2009b). We refer to that paper for any further details about models and results.…”
Section: Resultsmentioning
confidence: 99%
“…Dust shells with different temperatures were discovered by the detailed modelling of single D‐type SSs (e.g. Paper I; Angeloni et al 2007b; Contini et al 2009b).…”
Section: The Continuum Sedmentioning
confidence: 99%
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