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Photometric and spectroscopic studies of very low mass YSOs and young Brown Dwarfs in S106

Published online by Cambridge University Press:  01 August 2006

Yumiko Oasa
Yumiko Oasa*
Affiliation:
Graduate School of Science and Technology, Kobe University, 1-1 Rokko-dai, Nada-ku, Kobe, 657-8501, Japan email yummy@kobe-u.ac.jp
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Young brown dwarfs have been identified in a significant population in various star forming regions. Some deep surveys have yielded less massive objects with planetary-mass (e.g., Oasa et al. 1999; Lucas & Roche 2000). Nevertheless, it is not yet clear how abundant these very low-mass objects are formed. S106 is one of the nearest massive star-forming regions associated with prominent bipolar nebulae and an HII region. We have conducted near-infrared photometric and spectroscopic observations of very low-mass young stellar objects (YSOs) in the S106 region.

Keywords

star formationyoung brown dwarfnear-infrared observations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 457
Copyright
Copyright © International Astronomical Union 2007

References

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