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Detection of T-Tauri Star Candidates in the Canis Major Star-Forming Region and its Implications

Published online by Cambridge University Press:  04 August 2017

Suhardja D. Wiramihardja ,
Tomokazu Kogure ,
Makoto Nakano  and
Shigeomi Yoshida
Suhardja D. Wiramihardja
Affiliation:
Department of Astronomy, Faculty of Science, University of Kyoto, Kyoto 606, Japan
Tomokazu Kogure
Affiliation:
Department of Astronomy, Faculty of Science, University of Kyoto, Kyoto 606, Japan
Makoto Nakano
Affiliation:
Department of Astronomy, Faculty of Science, University of Kyoto, Kyoto 606, Japan
Shigeomi Yoshida
Affiliation:
Department of Astronomy, Faculty of Science, University of Kyoto, Kyoto 606, Japan

Extract

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We have made a survey of Hα-emission stars in the CMa R1 region with the 105cm Schmidt telescope at the Kiso Observatory. In an area of about 37 square degrees, a total of 107 Hα-emission stars (V = 6-15 mag.) was found, and, for all of them, the photographic photometry in the UBV system has been carried out.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 60
Copyright
Copyright © Reidel 1987 

References

Clariá, J.J.: 1974, Astron. J. 79, 1022.Google Scholar
Nakano, M., Yoshida, S., and Kogure, T.: 1984, Publ. Astron. Soc Japan, 36, 517.Google Scholar