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Near-IR imaging polarimetry of the RCW 106 cloud complex

Published online by Cambridge University Press:  03 March 2020

Shohei Tamaoki
Affiliation:
Nagoya City University, Graduate School of Natural Sciences Mizuho-cho, Mizuho-ku, Nagoya 467-8501, Japan
Koji Sugitani
Affiliation:
Nagoya City University, Graduate School of Natural Sciences Mizuho-cho, Mizuho-ku, Nagoya 467-8501, Japan
Takayoshi Kusune
Affiliation:
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mikata, Tokyo 181-8588, Japan
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Abstract

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We have carried out near-IR imaging polarimetry toward RCW 106 with the JHKs-simultaneous imaging polarimeter SIRPOL mounted on the IRSF 1.4m telescope at SAAO, in March and May, 2017 and January, 2018. We have observed 29 fields and covered mostly the southern part of the giant molecular cloud complex associated with the ${{\rm{H}}_\mathbb{I}}$ region RCW 106, which is located at a distance of 3.5 kpc (Moises etal 2011) and is elongated approximately in the north-south direction with a size of ∼70×15 pc. Our preliminary analysis indicates that the magnetic field seems to globally run along the complex elongation, unlike many other elongated clouds that are often reported to have their global elongations perpendicular to the magnetic fields. The RCW 106 complex consists of many small filaments or clumps. Some of such filaments seem to parallel to the magnetic fields, but some others perpendicular. Around the central part of the ${{\rm{H}}_\mathbb{I}}$ region RCW 106, the magnetic field appears to be influenced by the expansion of this ${{\rm{H}}_\mathbb{I}}$ region. Here, we present our preliminary results by comparing with the archival molecular line and far- to mid-IR data.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

References

Moises, A. P., Damineli, A., Figueredo, E., Blum, R. D., Conti, P. S., Barbosa, C. L., et al. 2011, MNRAS, 411, 705M CrossRefGoogle Scholar