hosokawa takashi

J-GLOBAL         Last updated: Dec 15, 2018 at 12:25
 
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Name
hosokawa takashi
E-mail
hosokwtkgmail.com
Affiliation
Kyoto University
Research funding number
30413967
ORCID ID
0000-0003-3127-5982

Academic & Professional Experience

 
Sep 2012
 - 
Jul 2016
Assistant professor, Department of physics, Faculty of science, The university of Tokyo
 
Mar 2011
 - 
Aug 2012
JSPS fellow for research abroad, NASA JPL
 
Apr 2010
 - 
Feb 2011
research associate, Department of physics, Faculty of science, Kyoto university
 
Apr 2007
 - 
Mar 2010
JSPS research fellow (PD), Division of Theoretical Astronomy, NAOJ
 
Apr 2005
 - 
Mar 2007
research associate, Division of Theoretical Astronomy, NAOJ
 

Published Papers

 
Monthly Notices of the Royal Astronomical Society      Aug 2018   [Refereed]
Accretion on to seed black holes (BHs) is believed to play a crucial role in formation of supermassive BHs observed at high-redshift (z > 6). Here, we investigate the combined effect of gas angular momentum and radiation feedback on the accreti...
Astronomy and Astrophysics      Aug 2018   [Refereed]
<BR /> Aims: We present the first simulations of the formation and feedback of massive stars which account for radiation forces as well as photoionization feedback (along with protostellar outflows). In two different accretion scenarios modeled, w...
The Astrophysical Journal      Jul 2018   [Refereed]
We conduct a theoretical study of the formation of massive stars over a wide range of metallicities from 10-5 to 1 {Z} and evaluate the star formation efficiencies (SFEs) from prestellar cloud cores taking into account mult...
The Astrophysical Journal      Jul 2018   [Refereed]
We report ALMA Cycle 3 observations in CO isotopes toward a dense core, MC27/L1521F in Taurus, which is considered to be at an early stage of multiple star formation in a turbulent environment. Although most of the high-density parts of this core ...
The Astrophysical Journal      Apr 2018   [Refereed]
Protoplanetary disks are thought to have lifetimes of several million yr in the solar neighborhood, but recent observations suggest that the disk lifetimes are shorter in a low-metallicity environment. We perform a suite of radiation hydrodynamics...