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19952004
most citedSupernova light curve models for the bump in the Optical Counterpart of X-Ray Flash 030723

32 citations · 32 across the 1 of their papers we have counts for

collaborators

10 papers

astro-ph200432 cited

Supernova light curve models for the bump in the Optical Counterpart of X-Ray Flash 030723

N. Tominaga, J. Deng, P. A. Mazzali +5

XRF 030723 is the first X-ray flash (XRF) to show in its optical light curve (LC) a bump that has been interpreted as the signature of a supernova (SN). After subtracting the after…

astro-ph2002

Hypernovae and their Nucleosynthesis

Ken'ichi Nomoto, Keiichi Maeda, Hideyuki Umeda +3

We review the characteristics of nucleosynthesis in 'Hypernovae', i.e., core-collapse supernovae with very large explosion energies ($ \gsim 10^{52} $ ergs). The hypernova yields s…

astro-ph2001

Hypernova Nucleosynthesis and Early Chemical Evolution

Ken'ichi Nomoto, Keiichi Maeda, Hideyuki Umeda

We review the characteristics of nucleosynthesis in 'Hypernovae', i.e., supernovae with very large explosion energies ($ \gsim 10^{52} $ ergs). The hypernova yields compared to tho…

astro-ph2001

Inhomogeneities in Newtonian Cosmology and its Backreaction to the Evolution of the Universe

Takayuki Tatekawa, Momoko Suda, Kei-ichi Maeda +1

We study an effect of inhomogeneity of density distribution of the Universe. We propose a new Lagrangian perturbation theory with a backreaction effect by inhomogeneity. The inhomo…

astro-ph2000

Explosive Nucleosynthesis in Aspherical Hypernova Explosions and Late Time Spectra of SN1998bw

K. Maeda, T. Nakamura, K. Nomoto +3

Aspherical explosion models for the hypernova (hyper-energetic supernova) SN 1998bw are presented. Nucleosynthesis in aspherical explosions is examined with a two-dimensional hydro…

gr-qc1999

Gravitational waves from a test particle scattered by a neutron star: Axial mode case

Kazuhiro Tominaga, Motoyuki Saijo, Kei-ichi Maeda

Using a metric perturbation method, we study gravitational waves from a test particle scattered by a spherically symmetric relativistic star. We calculate the energy spectrum and t…