activity
20032008
most citedThe Cassiopeia A Supernova was of Type IIB

324 citations · 1.5k across the 9 of their papers we have counts for

collaborators
Showing 2008Show all

6 papers · 1 filter

astro-ph2008213 cited

Tycho Brahe's 1572 supernova as a standard type Ia explosion revealed from its light echo spectrum

Oliver Krause, Masaomi Tanaka, Tomonori Usuda +4

Type Ia supernovae (SNe Ia) are thermonuclear explosions of white dwarf stars in close binary systems. They play an important role as cosmological distance indicators and have led…

astro-ph20081 cited

No Evidence for Variability of Intervening Absorption Lines toward GRB 060206: Implications for the Mg II Incidence Problem

Kentaro Aoki, Tomonori Totani, Takashi Hattori +6

We examine variability of absorption line strength of intervening systems along the line of sight to GRB 060206 at , by the low-resolution optical spectra obtained by the…

astro-ph2008126 cited

Strange filamentary structures ("fireballs") around a merger galaxy in the Coma cluster of galaxies

M. Yoshida, M. Yagi, Y. Komiyama +6

We found an unusual complex of narrow blue filaments, bright blue knots, and H-alpha emitting filaments and clouds, which morphologically resembled a complex of ``fireballs,'' exte…

astro-ph2008324 cited

The Cassiopeia A Supernova was of Type IIB

Oliver Krause, Stephan M. Birkmann, Tomonori Usuda +4

Cassiopeia A is one of the youngest supernova remnants known in the Milky Way and a unique laboratory for supernova physics. We present an optical spectrum of the Cassiopeia A supe…

astro-ph200817 cited

Integrated field spectroscopy of E+A (post-starburst) galaxies with the Kyoto3DII

Tomotsugu Goto, Atsushi Kawai, Atsushi Shimono +3

We have performed a two-dimensional spectroscopy of three nearby E+A (post-starburst) galaxies with the Kyoto3DII integral field spectrograph. In all the cases, Hdelta absorption i…

astro-ph2008248 cited

Asphericity in Supernova Explosions from Late-Time Spectroscopy

Keiichi Maeda, Koji Kawabata, Paolo A. Mazzali +15

Core-collapse supernovae (CC-SNe) are the explosions that announce the death of massive stars. Some CC-SNe are linked to long-duration gamma-ray bursts (GRBs) and are highly aspher…