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The CIDA Schmidt Objective-prism Survey: Fields in Taurus-Auriga and Ophiucus

Published online by Cambridge University Press:  12 April 2016

Cesar Briceño  and
Nuria Calvet
Cesar Briceño
Affiliation:
Centro de Investigaciones de Astronomía, Ap. P. 264, Mérida 5101-A, Venezuela
Nuria Calvet
Affiliation:
Centro de Investigaciones de Astronomía, Ap. P. 264, Mérida 5101-A, Venezuela

Abstract

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We have begun a deep objective prism Hα survey of starforming regions using the CIDA 1 m Schmidt Camera. We report here on the performance of the telescope for this kind of work, based on the study of selected areas in the Taurus-Auriga molecular clouds and the Ophiucus molecular clouds. Up to now seven plates taken in Taurus-Auriga have been visually scanned in a search for pre-main sequence candidates, with a coverage of about 120 square degrees over the whole complex, plus one plate taken in Ophiucus covering the entire cloud (≈ 18 square degrees).

Type
X. Stellar Astronomy
Information
International Astronomical Union Colloquium , Volume 148: The Future Utilisation of Schmidt Telescopes , 1995 , pp. 347 - 352
Copyright
Copyright © Astronomical Society of the Pacific 1995

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