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ASCA Observation of NGC1333 Star Forming Region

Published online by Cambridge University Press:  25 May 2016

M. Itoh
Affiliation:
Kobe University, Tsurukabuto, Nada, Kobe 657 Japan
H. Fukunaga
Affiliation:
Kobe University, Tsurukabuto, Nada, Kobe 657 Japan
K. Koyama
Affiliation:
Department of Physics, Graduate School of Science Kyoto University, Sakyo-ku, Kyoto 606-01 Japan
Y. Tsuboi
Affiliation:
Department of Physics, Graduate School of Science Kyoto University, Sakyo-ku, Kyoto 606-01 Japan
S. Yamauchi
Affiliation:
Faculty of Humanities and Social Sciences, Iwate University Ueda, Morioka, Iwate 020 Japan
N. Kobayashi
Affiliation:
National Astronomical Observatory Osawa, Mitaka, Tokyo, 181 Japan
M. Hayashi
Affiliation:
National Astronomical Observatory Osawa, Mitaka, Tokyo, 181 Japan
S. Ueno
Affiliation:
Department of Physics and Astronomy, University of Leicester Leicester, UK

Extract

The region south of the reflection nebula NGC1333 in Perseus is an active star forming region including numerous Herbig-Haro objects and at least 5 protostar candidates with molecular outflows and far-infrared emission. It has been actively studied in various wave bands (e.g. Aspin et al 1994 and references therein). We observed this region with ASCA with the primary objective to detect X-rays from the protostars embedded deep in the molecular cloud.

Type
Session 1: Plasma and Fresh Nucleosynthesis Phenomena
Copyright
Copyright © Kluwer 1998 

References

Aspin, C., Sandell, G., Russel, A.P.G., 1994, A&AS 106, 165 Google Scholar
Cernis, K., 1990, ApSS, 166, 315 Google Scholar
Preibisch, T. 1997, A&A, 324, 690 Google Scholar
Warin, S., et al., 1996, A&A, 306, 935 Google Scholar

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