Inferring Mass Loss Rates for Cool Luminous Stars from High-Resolution GHRS Spectra

Details Inferring Mass Loss Rates for Cool Luminous Stars from High-Resolution GHRS Spectra Inferring Mass Loss Rates for Cool Luminous Stars from High-Resolution GHRS Spectra

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000iaus..177..303l&link_type=gif

The Carbon Star Phenomenon, Proceedings of the 177th Symposium of the International Astronomical Union, held in Antalya, Turkey,

Astronomy and Astrophysics

Astronomy

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