NEW EVIDENCE FOR MASS LOSS FROM δ CEPHEI FROM H I 21 cm LINE OBSERVATIONS

Recently published Spitzer Space Telescope observations of the classical Cepheid archetype δ Cephei revealed an extended dusty nebula surrounding this star and its hot companion HD 213307. At far-infrared wavelengths, the emission resembles a bow shock aligned with the direction of space motion of t...

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Bibliographic Details
Main Authors: Marengo, Massimo (Author), Evans, N. R. (Author), Bono, G. (Author), Matthews, Lynn D. (Contributor)
Other Authors: Haystack Observatory (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2015-02-20T20:07:56Z.
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