Abstract
Using IR Camera of PtSi array, we have started to take the near infrared images of molecular clouds that are forming stars. In this paper, we present the preliminary results of detecting the infrared sources possibly embedded in the molecular clouds. These embedded sources can be the protostellar cluster.
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Hayashi, M., and Murata, Y.: 1992, PASJ ,44, 391
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© 1994 Springer Science+Business Media Dordrecht
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Hayashi, S.S., Ueno, M. (1994). Characteristics of the Infrared Clusters in Various Scale Molecular Clouds. In: McLean, I.S. (eds) Infrared Astronomy with Arrays. Astrophysics and Space Science Library, vol 190. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1070-9_22
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DOI: https://doi.org/10.1007/978-94-011-1070-9_22
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-4466-0
Online ISBN: 978-94-011-1070-9
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