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Structure and kinematics in the northeastern outer parts of the SMC

Published online by Cambridge University Press:  19 July 2016

D. Hatzidimitriou ,
R. D. Cannon  and
M.R.S. Hawkins
D. Hatzidimitriou
Affiliation:
Anglo-Australian Observatory, Epping, NSW 2121, Australia
R. D. Cannon
Affiliation:
Anglo-Australian Observatory, Epping, NSW 2121, Australia
M.R.S. Hawkins
Affiliation:
Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, Scotland

Abstract

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We present preliminary results from a study of the radial velocities of red horizontal branch stars in the north-eastern outer parts of the Small Magellanic Cloud (SMC). The sample is located in an area with a large line-of-sight depth of 15 kpc. It is suggested that there is a correlation between line-of-sight distance and radial velocity for these stars, with the more distant ones showing significantly higher velocities.

Type
Large-Scale Structure and Kinematics
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 107 - 108
Copyright
Copyright © Kluwer 1991 

References

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