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Star Formation at Large Galactic z?

Published online by Cambridge University Press:  03 August 2017

William Tobin
William Tobin*
Affiliation:
Department of Physics and Mt John University Observatory, University of Canterbury, Christchurch 1, New Zealand

Abstract

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It seems very probable that young, luminous B stars occur in the galactic halo. An origin in the disc followed by ejection may account for many of these stars; certain proposed formation-ejection mechanisms involve the infall of halo material. The kinematics and supposed locations of some halo B stars seem incompatible with an origin in the disc, suggesting that these stars may have formed in the halo.

Type
I. The Disk-Halo Interface in Our Galaxy
Information
Symposium - International Astronomical Union , Volume 144: The Interstellar Disk-Halo Connection in Galaxies , 1991 , pp. 109 - 119
Copyright
Copyright © Kluwer 1991 

References

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