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The evaporation of spherical clouds in a hot gas. I - Classical and saturated mass loss rates
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The evaporation of spherical clouds in a hot gas. I - Classical and saturated mass loss rates
The evaporation of spherical clouds in a hot gas. I - Classical and saturated mass loss rates
LC
L. L. Cowie
L. L. Cowie
CM
C. F. McKee
C. F. McKee
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1 January 1977
journal article
Published by
American Astronomical Society
in
The Astrophysical Journal
Vol. 211
,
135-146
https://doi.org/10.1086/154911
Abstract
No abstract available
Keywords
EVAPORATION
HIGH TEMPERATURE GASES
INTERSTELLAR GAS
NEBULAE
SUPERNOVA REMNANTS
CONDUCTIVE HEAT TRANSFER
HEAT FLUX
MASS FLOW RATE
SOLAR WIND
TEMPERATURE PROFILES
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