Oxygen-rich mass loss from carbon-rich stars - Some implicationsThe degree of dust-to-gas coupling in the atmospheres of red giant stars is evaluated, and nonzero drift velocities are found. Chemical fractionation of the stellar atmosphere on an evolutionary time scale is implied.
Document ID
19900044817
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Stencel, Robert E. (Colorado Univ. Boulder, CO, United States)
Pesce, Joseph E. (Colorado, University Boulder, United States)