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Summary Introduction

Published online by Cambridge University Press:  19 March 2018

A. Deutsch
A. Deutsch*
Affiliation:
Mt. Wilson and Palomar Observatories

Extract

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Gas can be observed to flow from a wide variety of stars into the interstellar medium, and to do so in a fascinating variety of ways. In some flows, the temperature exceeds a million degrees; in others, it cannot be distinguished from zero. Flow velocities range from 5 000 km/s down to one or two km/s at the limit of detection. The particle densities in some flows are at least 109 times larger than in others. The rates of mass-loss span the range from zero to probably more than 1026 g/s.

Information

Type
Part III. Spherically-Symmetric Motions in Stellar Atmospheres
Information
Symposium - International Astronomical Union , Volume 12: Aerodynamic Phenomena in Stellar Atmospheres , 1960, pp. 238 - 259
Copyright
Copyright © Italian physical society 1960 

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