output
19972026
most citedHI4PI: A full-sky HI survey based on EBHIS and GASS

1.6k citations

Showing 2018Show all

51 papers · 1 filter

astro-ph.SR2018★ 27 cited

Dependence of Hall Coefficient on Grain Size and Cosmic Ray Rate and Implication for Circumstellar Disk Formation

Shunta Koga, Yusuke Tsukamoto, Satoshi Okuzumi +1

The Hall effect plays a significant role in star formation because it induces rotation in the infalling envelope, which in turn affects the formation and evolution of the circumste…

astro-ph.GA2018★ 4 cited

Magneto Rotational Instability in Magnetized AGN Tori

Yuki Kudoh, Keiichi Wada

It is widely believed that in active galactic nuclei (AGNs) a supermassive black hole with an accretion disk is surrounded by an optically and geometrically thick torus at sub-pars…

astro-ph.GA2018★ 6 cited

A 1000 AU Scale Molecular Outflow Driven by a Protostar with an age of <4000 Years

Ray S. Furuya, Yoshimi Kitamura, Hiroko Shinnaga

To shed light on the early phase of a low-mass protostar formation process, we conducted interferometric observations towards a protostar GF9-2 using the CARMA and SMA. The observa…

astro-ph.GA2018★ 63 cited

JCMT BISTRO survey: Magnetic Fields within the Hub-Filament Structure in IC 5146

Jia-Wei Wang, Shih-Ping Lai, Chakali Eswaraiah +130

We present the 850 m polarization observations toward the IC5146 filamentary cloud taken using the Submillimetre Common-User Bolometer Array 2 (SCUBA-2) and its associated polar…

astro-ph.SR2018★ 40 cited

Does misalignment between magnetic field and angular momentum enhance or suppress circumstellar disk formation?

Y. Tsukamoto, S. Okuzumi, K. Iwasaki +2

The effect of misalignment between the magnetic field $\magB$ and the angular momentum $\Jang$ of molecular cloud cores on the angular momentum evolution during the gravitational c…

astro-ph.GA2018★ 3 cited

Radio broadband visualization of global three-dimensional magneto-hydrodynamical simulations of spiral galaxies II. Faraday Depolarization from 100MHz to 10GHz

Mami Machida, Takuya Akahori, Kenji Nakamura +2

Observational study of galactic magnetic fields is limited by projected observables. Comparison with numerical simulations is helpful to understand the real structures, and observa…