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Star Formation at High Galactic Latitude: A Case for Extensions to the Hα Survey

Published online by Cambridge University Press:  16 May 2016

Kristen A. Larson
Kristen A. Larson*
Affiliation:
Department of Physics, Applied Physics & Astronomy, Rensselaer Polytechnic Institute, Troy, NY 12180, USA; kal@charon.phys.rpi.edu
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Abstract

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The AAO/UKST Hα Survey should be extended to high Galactic latitude (∣b∣ > 25°) to search for T Tauri stars. The Hα Survey can contribute to a complete inventory of young stellar objects in high-latitude clouds, which will help define the limits of conditions and processes that lead to star formation.

Keywords

ISM: cloudsstars: emission-linestars: pre-main sequencesurveys
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 15 , Issue 1 , 1998 , pp. 155 - 156
Copyright
Copyright © Astronomical Society of Australia 1998

References

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