Mass loss from the infrared star CIT 6

Details Mass loss from the infrared star CIT 6 Mass loss from the infrared star CIT 6

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...202..183m&link_type=abstract

Astrophysical Journal, vol. 202, Nov. 15, 1975, pt. 1, p. 183-190.

Mathematics

35

Carbon Monoxide, Infrared Stars, Interstellar Masers, Interstellar Matter, Stellar Mass Ejection, Brightness Temperature, Cosmic Dust, Emission Spectra, Stellar Evolution, Stellar Luminosity, Stellar Spectra

Scientific paper

2.6 mm carbon monoxide emission from a small region surrounding CIT 6 is
observed. The line profiles are doubly peaked and interpreted as arising
from a disk which is rotationally ejected from the outer layers of the
stellar atmosphere. The mathematics of rotationally forced ejection are
presented.

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