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Evidence For Cloud-Cloud Collision and Parsec-Scale Stellar Feedback Within the L1641-N Region
Fumitaka Nakamura, Tomoya Miura, Yoshimi Kitamura +7
We present high spatial resolution CO () images taken by the Nobeyama 45m telescope toward a area including the L1641-N cluster. The effective spatia…
Complex Scattered Radiation Fields and Multiple Magnetic Fields in the Protostellar Cluster in NGC 2264
Jungmi Kwon, Motohide Tamura, Ryo Kandori +9
Near-infrared (IR) imaging polarimetry in the J, H, and Ks bands has been carried out for the protostellar cluster region around NGC 2264 IRS 2 in the Monoceros OB1 molecular cloud…
Clustered Star Formation in Magnetic Clouds: Properties of Dense Cores Formed in Outflow-Driven Turbulence
Fumitaka Nakamura, Zhi-Yun Li
We investigate the physical properties of dense cores formed in turbulent, magnetized, parsec-scale clumps of molecular clouds, using three-dimensional numerical simulations that i…
Magnetic Flux Expulsion in Star Formation
Bo Zhao, Zhi-Yun Li, Fumitaka Nakamura +2
Stars form in dense cores of magnetized molecular clouds. If the magnetic flux threading the cores is dragged into the stars, the stellar field would be orders of magnitude stronge…
Molecular Outflows From the Protocluster, Serpens South
Fumitaka Nakamura, Koji Sugitani, Yoshito Shimajiri +8
We present the results of CO () and HCO () mapping observations toward a nearby embedded cluster, Serpens South, using the ASTE 10 m telescope. Our CO () m…
Near-Infrared Imaging Polarimetry Toward Serpens South: Revealing the Importance of the Magnetic Field
K. Sugitani, F. Nakamura, M. Watanabe +9
The Serpens South embedded cluster, which is located at the constricted part in a long filamentary infrared dark cloud, is believed to be in very early stage of cluster formation.…