Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-10T06:42:17.031Z Has data issue: false hasContentIssue false

He abundance in red giants

Published online by Cambridge University Press:  07 August 2017

J.A. de Freitas Pacheco
Affiliation:
Instituto Astronômico e Geofísico, Universidade de SÃo Paulo, Brazil
R.D.D. Costa
Affiliation:
Instituto Astronômico e Geofísico, Universidade de SÃo Paulo, Brazil

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.

The He abundance in red giants is not well known. Moreover, some He enhancement in the stellar atmospheres is expected to occur as a consequence of distinct dredge-up episodes. In the present work is reported and discussed the He abundance for 5 symbiotic nebulae (Hen 2-38, RR Tel, RX Pup, HM Sge, KX TrA). Self-absorption effects in both hydrogen and HeI lines were taken into account.

Type
Poster Papers
Copyright
Copyright © Kluwer 

References

Almog, Y. and Netzer, H. (1989) Mon. Not. R. astr. Soc. 238, 57.Google Scholar
De Freitas Pacheco, J.A. and Costa, R.D.D. (1991a) - submitted to publication.Google Scholar
Netzer, H. (1975) Mon. Not. R. astr. Soc. 171, 395.CrossRefGoogle Scholar