activity
20032008
most citedThe Unique Type Ib Supernova 2005bf at Nebular Phases: A Possible Birth Event of A Strongly Magnetized Neutron Star

221 citations · 438 across the 4 of their papers we have counts for

collaborators

8 papers

astro-ph200883 cited

Early Formation of Dust in the Ejecta of Type Ib SN 2006jc and Temperature and Mass of the Dust

T. Nozawa, T. Kozasa, N. Tominaga +8

SN 2006jc is a peculiar supernova (SN), in which the formation of dust has been confirmed at an early epoch of ~50 days after the explosion. We investigate the possibility of such…

astro-ph2007221 cited

The Unique Type Ib Supernova 2005bf at Nebular Phases: A Possible Birth Event of A Strongly Magnetized Neutron Star

K. Maeda, M. Tanaka, K. Nomoto +6

Late phase nebular spectra and photometry of Type Ib Supernova (SN) 2005bf taken by the Subaru telescope at ~ 270 and ~ 310 days since the explosion are presented. Emission lines (…

astro-ph200674 cited

Asymmetric Explosion of Type Ia Supernovae as Seen from Near Infrared Observations

K. Motohara, K. Maeda, C. L. Gerardy +8

We present near-infrared spectra of late phase (>200 d) Type Ia supernovae (SNe Ia) taken at the Subaru telescope. The [Fe II] line of SN 2003hv shows a clear flat-topped feature,…

astro-ph200660 cited

The Optical/Near-Infrared Light Curves of SN 2002ap for the First 1.5 Years after Discovery

Hiroyuki Tomita, Jinsong Deng, Keiichi Maeda +9

Late-time BVRIJHK photometry of the peculiar Type Ic SN 2002ap, taken between 2002 June 12 and 2003 August 29 with the MAGNUM telescope, is presented. The light curve decline rate…

astro-ph2005

Optical Emission from Aspherical Supernovae and the Hypernova SN 1998bw

K. Maeda, P. A. Mazzali, K. Nomoto

A fully 3D Monte Carlo scheme is applied to compute optical bolometric light curves for aspherical (jet-like) supernova explosion models. Density and abundance distributions are ta…

astro-ph2005

Core-Collapse Very Massive Stars: Evolution, Explosion, and Nucleosynthesis of Population III 500 -- 1000 Stars

T. Ohkubo, H. Umeda, K. Maeda +4

We calculate evolution, collapse, explosion, and nucleosynthesis of Population III very-massive stars with 500 and 1000. Presupernova evolution is calculated…