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ISO LWS spectra of AGB and post-AGB objects

Published online by Cambridge University Press:  25 May 2016

P. Cox
P. Cox*
Affiliation:
Institut d'Astrophysique Spatiale, Bât 121, Université de Paris XI, 91405 Orsay Cedex, France

Abstract

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We present ISO Long Wavelength Spectrometer (LWS) grating spectra of AGB and post-AGB stars. The LWS instrument and the calibration procedures are described by Clegg et al. (1996) and Swinyard et al. (1996).

Type
ISO First Results
Information
Symposium - International Astronomical Union , Volume 178: Molecules in Astrophysics: Probes and Processes , 1997 , pp. 389 - 392
Copyright
Copyright © Kluwer 1997 

References

Barlow, M.J., Nguyen-Q-Rieu, , Truong-Bach, , Cernicharo, J. et al 1996, A&A 315, L241.Google Scholar
Cernicharo, J., Barlow, M.J., Cox, P., González-Alfonso, E., et al. 1996, A&A 315, L201.Google Scholar
Clegg, P.E. et al. 1996, A&A 315, L38.Google Scholar
Cox, P., González-Alfonso, E., Barlow, M.J., Liu, X.-W. et al. 1996, A&A 315, L265.Google Scholar
Liu, X.-W., Barlow, M.J., Nguyen-Q-Rieu, , Truong-Bach, , et al. 1996, A&A 315, L257.Google Scholar
Swinyard, B.M. et al. 1996, A&A 315, L43.Google Scholar