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Stellar outflow: relative motions of nebulae and of stars

Published online by Cambridge University Press:  14 August 2015

Beverly T. Lynds
Beverly T. Lynds*
Affiliation:
Kitt Peak National Observatory1

Extract

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On the basis of arguments presented by Roberts (1972) and of Shu et al. (1972), Minn and Greenberg (1973) argued that the velocity differences between newly formed hot stars and the surrounding interstellar medium are sufficiently different so that typical H II regions should consist of material which is continually being replaced by the ambient medium and which should therefore possess the velocity of the medium rather than that of the star. Obviously, the critical test of this hypothesis will be a comparison of nebular velocities with the velocities of the exciting stars.

Type
Session 1: Optical Spectroscopy
Information
Symposium - International Astronomical Union , Volume 83: Mass Loss and Evolution of O-Type Stars , 1979 , pp. 55 - 57
Copyright
Copyright © Reidel 1979 

References

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