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20022011
most citedSuperconductivity at 27 K in tetragonal FeSe under high pressure

718 citations

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16 papers · 1 filter

astro-ph20087 cited

Microstructure and kinematics of H2O masers in the massive star forming region IRAS 06061+2151

K. Motogi, Y. Watanabe, K. Sorai +14

We have made multi-epoch VLBI observations of H2O maser emission in the massive star forming region IRAS 06061+2151 with the Japanese VLBI network (JVN) from 2005 May to 2007 Octob…

astro-ph200840 cited

Suzaku broad-band spectroscopy of RX J1347.5-1145: constraints on the extremely hot gas and non-thermal emission

N. Ota, K. Murase, T. Kitayama +6

We present the results from the analysis of long Suzaku observations of the most X-ray luminous galaxy cluster RX J1347.5-1145 at z=0.451. Aims: We study physical properties of the…

astro-ph2008

The Impact of a Supernova Explosion in a Very Massive Binary

Jun'ichi Sato, Masayuki Umemura, Keisuke Sawada

We consider the effect of a supernova (SN) explosion in a very massive binary that is expected to form in a portion of Population III stars with the mass higher than 100.…

astro-ph200830 cited

Extinction curves flattened by reverse shocks in supernovae

Hiroyuki Hirashita, Takaya Nozawa, Tsutomu T. Takeuchi +1

We investigate the extinction curves of young galaxies in which dust is supplied from Type II supernovae (SNe II) and/or pair instability supernovae (PISNe). Since at high redshift…

astro-ph200746 cited

Nuclear/Circumnuclear Starbursts and Active Galactic Nuclei Mass Accretion in Seyfert Galaxies

Yasuyuki Watabe, Nozomu Kawakatu, Masatoshi Imanishi

We investigated the correlation between nuclear/circumnuclear starbursts around the active galactic nuclei (AGNs) and the AGN activities for 43 Seyfert galaxies in the CfA and 12 m…

astro-ph200711 cited

Fragment-collision model for compound chondrule formation: Estimation of collision probability

Hitoshi Miura, Seiji Yasuda, Taishi Nakamoto

We propose a new scenario for compound chondrule formation named as "fragment-collision model," in the framework of the shock-wave heating model. A molten cm-sized dust particle (p…