scholarly journals NEAR-INFRARED IMAGING POLARIMETRY OF THE SERPENS CLOUD CORE: MAGNETIC FIELD STRUCTURE, OUTFLOWS, AND INFLOWS IN A CLUSTER FORMING CLUMP

2010 ◽  
Vol 716 (1) ◽  
pp. 299-314 ◽  
Author(s):  
Koji Sugitani ◽  
Fumitaka Nakamura ◽  
Motohide Tamura ◽  
Makoto Watanabe ◽  
Ryo Kandori ◽  
...  
2016 ◽  
Vol 824 (2) ◽  
pp. 95 ◽  
Author(s):  
Jungmi Kwon ◽  
Motohide Tamura ◽  
James H. Hough ◽  
Tetsuya Nagata ◽  
Nobuhiko Kusakabe ◽  
...  

2011 ◽  
Vol 734 (1) ◽  
pp. 63 ◽  
Author(s):  
K. Sugitani ◽  
F. Nakamura ◽  
M. Watanabe ◽  
M. Tamura ◽  
S. Nishiyama ◽  
...  

2018 ◽  
Vol 234 (2) ◽  
pp. 42 ◽  
Author(s):  
Jungmi Kwon ◽  
Takao Nakagawa ◽  
Motohide Tamura ◽  
James H. Hough ◽  
Minho Choi ◽  
...  

2009 ◽  
Vol 137 (2) ◽  
pp. 3149-3157 ◽  
Author(s):  
Hiro Saito ◽  
Motohide Tamura ◽  
Ryo Kandori ◽  
Nobuhiko Kusakabe ◽  
Jun Hashimoto ◽  
...  

2000 ◽  
Vol 536 (2) ◽  
pp. L89-L92 ◽  
Author(s):  
Joel Silber ◽  
Tim Gledhill ◽  
Gaspard Duchêne ◽  
François Ménard

2009 ◽  
Vol 708 (1) ◽  
pp. 758-769 ◽  
Author(s):  
Jungmi Kwon ◽  
Minho Choi ◽  
Soojong Pak ◽  
Ryo Kandori ◽  
Motohide Tamura ◽  
...  

1997 ◽  
Vol 112 (1) ◽  
pp. 109-191 ◽  
Author(s):  
Mary Barsony ◽  
Scott J. Kenyon ◽  
Elizabeth A. Lada ◽  
Peter J. Teuben

2013 ◽  
Vol 772 (2) ◽  
pp. 145 ◽  
Author(s):  
Michihiro Takami ◽  
Jennifer L. Karr ◽  
Jun Hashimoto ◽  
Hyosun Kim ◽  
John Wisniewski ◽  
...  

1991 ◽  
Vol 248 (4) ◽  
pp. 715-729 ◽  
Author(s):  
N. R. Minchin ◽  
J. H. Hough ◽  
A. McCall ◽  
M. G. Burton ◽  
M. J. McCaughrean ◽  
...  

2008 ◽  
Vol 4 (S259) ◽  
pp. 97-98 ◽  
Author(s):  
Nobuhiko Kusakabe ◽  
Motohide Tamura ◽  
Ryo Kandori ◽  

AbstractMagnetic fields are believed to play an important role in star formation. We observed M42 and Mon R2 massive star forming regions using the wide-field (8′ × 8′) near-infrared imaging polarimeter SIRPOL in South Africa. Magnetic fields are mapped on the basis of dichroic polarized light from hundreds of young stars embedded in the regions. We found “hourglass shaped” magnetic field structure toward OMC-1 region, which is very consistent with magnetic fields traced by using dust emission polarimetry at sub-mm to FIR wavelengths. In the Mon R2 region, we found “S-shaped” magnetic field structure across the massive protostar IRS 1 and IRS 2. We will present the results of comparison of magnetic fields at NIR with those at other wavelengths.


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