Mass loss from evolved stars - Response to a review by Zuckerman (1987)

Details Mass loss from evolved stars - Response to a review by Zuckerman (1987) Mass loss from evolved stars - Response to a review by Zuckerman (1987)

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100.1446t&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, Nov. 1988, p. 1446-1451.

Astronomy and Astrophysics

Astronomy

4

Color-Color Diagram, Infrared Stars, Late Stars, Stellar Mass Ejection, Astronomical Photometry, Carbon Stars, Infrared Spectra, Oxygen

Scientific paper

We comment on a recent negative review by Zuckerman (1987) of an earlier paper of ours on the interpretation of infrared emission from highly-evolved stars (Thronson et al. 1987). Many of his criticisms are based on apparent misreadings or misunderstandings of our paper, which we here attempt to correct. In addition we discuss the use of mid- and far-infrared color-color diagrams to study mass-losing stars and repeat some of the warnings that might not have been sufficiently clear in our previous paper. We also discuss the analysis of Thronson et al. in light of more-recent published work.

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