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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…
The Origin of OB Clusters: From 10 pc to 0.1 pc
Hauyu Baobab Liu, Guillermo Quintana-Lacaci, Ke Wang +4
We observe the 1.2 mm continuum emission around the OB cluster forming region G10.6-0.4, using the IRAM 30m telescope MAMBO-2 bolometer array and the Submillimeter array. Compariso…
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…
Nonideal MHD Effects and Magnetic Braking Catastrophe in Protostellar Disk Formation
Zhi-Yun Li, Ruben Krasnopolsky, Hsien Shang
Dense, star-forming, cores of molecular clouds are observed to be significantly magnetized. A realistic magnetic field of moderate strength has been shown to suppress, through cata…
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…
Disk Formation in Magnetized Clouds Enabled by the Hall Effect
Ruben Krasnopolsky, Zhi-Yun Li, Hsien Shang
Stars form in dense cores of molecular clouds that are observed to be significantly magnetized. A dynamically important magnetic field presents a significant obstacle to the format…