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Volumn 477, Issue 2 PART I, 1997, Pages 926-939

Deriving the geometry of be star circumstellar envelopes from continuum spectropolarimetry. I. The case of ζ tauri

Author keywords

Circumstellar matter; Polarization; Radiative transfer; Stars: emission line, Be; Stars: individual ( Tauri)

Indexed keywords


EID: 21744442838     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/303747     Document Type: Article
Times cited : (92)

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