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1998•Symposium - International Astronomical UnionOpen access

ASCA Observation of NGC1333 Star Forming Region

Mitsumasa Itoh, H. Fukunaga, Kazuya Koyama, Yuka Tsuboi, Sanae Yamauchi, N. Kobayashi, Masahiko Hayashi, Satoru Ueno

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Abstract

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.

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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.

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Available abstract

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.

Key concepts: Protostar, Reflection nebula, Physics, Astrophysics, Herbig–Haro object, Molecular cloud, Nebula, Star (game theory)

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