Mass loss in red giants and supergiants

Details Mass loss in red giants and supergiants Mass loss in red giants and supergiants

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...204l..41s&link_type=abstract

Astrophysical Journal, vol. 204, Feb. 15, 1976, pt. 2, p. L41-L45.

Astronomy and Astrophysics

Astrophysics

11

Giant Stars, Late Stars, Mass Transfer, Stellar Envelopes, Stellar Spectrophotometry, Supergiant Stars, Graphs (Charts), M Stars, Mass Flow Rate, Optical Resonance, Photoelectric Emission, Stellar Luminosity

Scientific paper

The circumstellar envelopes surrounding 13 late-type giants and supergiants have been studied using a homogeneous collection of high-resolution, photoelectric scans of strong optical resonance lines. Various properties of the envelopes, including the mass loss rate, dilution factor, hydrogen density, and degree of ionization, have been determined quantitatively.

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