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IRSF/SIRIUS near-infrared survey of the Magellanic Clouds: triggered star formation in N11 in the Large Magellanic Cloud

Published online by Cambridge University Press:  01 August 2006

H. Hatano ,
R. Kadowaki ,
D. Kato  and
S. Sato
H. Hatano
Affiliation:
Department of Astrophysics, Nagoya University, Chikusa-ku, Nagoya 464-8602, Japan email: hattan@z.phys.nagoya-u.ac.jp.
R. Kadowaki
Affiliation:
Department of Astrophysics, Nagoya University, Chikusa-ku, Nagoya 464-8602, Japan email: hattan@z.phys.nagoya-u.ac.jp.
D. Kato
Affiliation:
Department of Astrophysics, Nagoya University, Chikusa-ku, Nagoya 464-8602, Japan email: hattan@z.phys.nagoya-u.ac.jp.
S. Sato
Affiliation:
Department of Astrophysics, Nagoya University, Chikusa-ku, Nagoya 464-8602, Japan email: hattan@z.phys.nagoya-u.ac.jp.
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Abstract

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A near-infrared survey of the Magellanic Clouds has been carried out with IRSF/SIRIUS. As a part of the results, we present a study of triggered star formation in N11 in the LMC.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 423
Copyright
Copyright © International Astronomical Union 2007

References

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