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2018ApJ...859...29N - Astrophys. J., 859, 29-29 (2018/May-3)

Magnetohydrodynamic simulations of a plunging black hole into a molecular cloud.

NOMURA M., OKA T., YAMADA M., TAKEKAWA S., OHSUGA K., TAKAHASHI H.R. and ASAHINA Y.

Abstract (from CDS):

Using two-dimensional magnetohydrodynamic simulations, we investigated the gas dynamics around a black hole (BH) plunging into a molecular cloud. In these calculations, we assumed a parallel-magnetic-field layer in the cloud. The size of the accelerated region is far larger than the Bondi-Hoyle-Lyttleton radius, being approximately inversely proportional to the Alfven Mach number for the plunging BH. Our results successfully reproduce the "Y" shape in position-velocity maps of the "Bullet" in the W44 molecular cloud. The size of the Bullet is also reproduced within an order of magnitude using a reasonable parameter set. This consistency supports the shooting model of the Bullet, according to which an isolated BH plunged into a molecular cloud to form a compact broad-velocity-width feature.

Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.

Journal keyword(s): ISM: clouds - ISM: kinematics and dynamics - magnetohydrodynamics MHD - methods: numerical

Simbad objects: 3

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