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Spectroscopic study of stars with dusty disks

Published online by Cambridge University Press:  26 May 2016

T. Sivarani
Affiliation:
Indian Institute of Astrophysics, Bangalore, India
M. Parthasarathy
Affiliation:
Indian Institute of Astrophysics, Bangalore, India

Abstract

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We have selected several stars with far-IR (IRAS) fluxes indicating the presence of circumstellar dust shells and disks. In this paper we present an analysis of the spectra of these stars. In several of these stars we find evidence for gaseous envelopes in addition to dusty disks. In some of these stars we find complex and variable Ha profiles indicating the variations in the circumstellar envelopes and disks.

Type
Part IV: Protoplanetary and β Pic disks
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Jura, M., & Turner, J., 1998, Nature. 395, 144.CrossRefGoogle Scholar
Aumann, H.H., Gillett, F.C., Beichmann, C.A., de Jong, T., Houch, J.R., Low, F.J., Neugebauer, G., Walker, R.G., & Wesselius, P.R. 1984, ApJ, 278, L23.CrossRefGoogle Scholar
Backman, D., & Paresce, F. 1993, in Protostars & Planets III (eds Levy, E.H., Lunine, J., 1253 (Univ. Arizona Press, Tucson)Google Scholar
Zuckerman, B., & Dyck, H.M. 1986, ApJ, 311, 3450.CrossRefGoogle Scholar