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Envelope Activity of the K-Type Supergiant HD 4817

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Activity in Cool Star Envelopes

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 143))

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Abstract

The metallic emission line Cal 6572.8 Å was detected as variable in intensity in the high dispersion spectra collected at the Dominion Astrophysical Observatory, Victoria, Canada. The radial velocity of this line is about −35 km/s relative to the photospheric absorption lines. It indicates the existence of a gas expanding envelope around this star.

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© 1988 Kluwer Academic Publishers

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Smoliński, J., Climenhaga, J.L. (1988). Envelope Activity of the K-Type Supergiant HD 4817. In: Havnes, O., Pettersen, B.R., Schmitt, J.H.M.M., Solheim, J.E. (eds) Activity in Cool Star Envelopes. Astrophysics and Space Science Library, vol 143. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2951-7_50

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  • DOI: https://doi.org/10.1007/978-94-009-2951-7_50

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-7827-6

  • Online ISBN: 978-94-009-2951-7

  • eBook Packages: Springer Book Archive

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