Hostname: page-component-77c89778f8-swr86 Total loading time: 0 Render date: 2024-07-19T23:29:33.673Z Has data issue: false hasContentIssue false

Circumstellar CA II K Lines in G, K and M Giants and Supergiants

Published online by Cambridge University Press:  08 February 2017

A. H. Vaughan Jr.
Affiliation:
Mt.Wilson and Palomar Observatories, California Institute of Technology and Carnegie Institute of Washington, Pasadena, California
A. Skumanich
Affiliation:
Mt.Wilson and Palomar Observatories, California Institute of Technology and Carnegie Institute of Washington, Pasadena, California

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Tentative evidence, based on photoelectric observations of the Ca+ emission core, is presented for the existence of circumstellar envelopes in several G and K type “giants.” A significant emission asymmetry in α Tau may imply a chromospheric rather than a circumstellar source.

Type
Part C
Copyright
Copyright © 1970

References

Deutsch, A. J. 1960, Stellar Atmospheres: Stars and Stellar Systems, VI, ed. Greenstein, J. L. (Chicago: Univ. of Chicago Press), p. 543.Google Scholar
Hummer, D. G., and Rybicki, G. B. 1968, Ap. J., 153, L107.Google Scholar
Vaughan, A. H. Jr. 1968, Ap. J., 154, 87.Google Scholar
Weyman, R., 1963, Ann. Rev. Astr. and Ap., 1, 97.Google Scholar
Wilson, O. C., and Bappu, M. K. V. 1957, Ap. J., 125, 661.Google Scholar
Wilson, O. C. 1960, Ap. J., 132, 136.Google Scholar