most citedThe metamorphosis of Supernova SN2008D/XRF080109: a link between Supernovae and GRBs/Hypernovae

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astro-ph200842 cited

Optical photometry and spectroscopy of the type Ibn supernova SN 2006jc until the onset of dust formation

G. C. Anupama, D. K. Sahu, U. K. Gurugubelli +4

We present optical UBVRI photometric and spectroscopic data of the type Ibn supernova SN 2006jc, until the onset of the dust forming phase. The optical spectrum shows a blue contin…

astro-ph200860 cited

Injection of Short-Lived Radionuclides into the Early Solar System from a Faint Supernova with Mixing-Fallback

A. Takigawa, J. Miki, S. Tachibana +4

Several short-lived radionuclides (SLRs) were present in the early solar system, some of which should have formed just prior to or soon after the solar system formation. Stellar nu…

astro-ph2008258 cited

The metamorphosis of Supernova SN2008D/XRF080109: a link between Supernovae and GRBs/Hypernovae

Paolo A. Mazzali, Stefano Valenti, Massimo Della Valle +38

The only supernovae (SNe) to have shown early gamma-ray or X-ray emission thus far are overenergetic, broad-lined Type Ic SNe (Hypernovae - HNe). Recently, SN 2008D shows several n…

astro-ph200831 cited

Optical Spectropolarimetry and Asphericity of Type Ic SN 2007gr

Masaomi Tanaka, Koji S. Kawabata, Keiichi Maeda +2

We present optical spectropolarimetric observations of Type Ic supernova (SN) 2007gr with Subaru telescope at 21 days after the maximum brightness (~37 days after the explosion). N…

astro-ph2008

The Connection between Gamma-Ray Bursts and Extremely Metal-Poor Stars as Nucleosynthetic Probes of the Early Universe

K. Nomoto, N. Tominaga, M. Tanaka +2

The connection between the long GRBs and Type Ic Supernovae (SNe) has revealed the interesting diversity: (i) GRB-SNe, (ii) Non-GRB Hypernovae (HNe), (iii) X-Ray Flash (XRF)-SNe, a…

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…