Type Ib supernova 2008D associated with the luminous X-ray transient 080109: An energetic explosion of a massive helium star

Masaomi Tanaka, Nozomu Tominaga, Ken'ichi Nomoto, S. Valenti, D. K. Sahu, T. Minezaki, Y. Yoshii, M. Yoshida, G. C. Anupama, S. Benetti, G. Chincarini, M. Della Valle, P. A. Mazzali, E. Pian

研究成果: Article査読

68 被引用数 (Scopus)

抄録

We present a theoretical model for supernova SN 2008D associated with the luminous X-ray transient 080109. The bolometric light curve and optical spectra of the SN are modeled based on the progenitor models and the explosion models obtained from hydrodynamic/nucleosynthetic calculations. We find that SN 2008D is a more energetic explosion than normal core-collapse supernovae, with an ejecta mass of Mej = 5.3 ± 1.0M and a kinetic energy of EK = 6.0 ± 2.5 × 1051 erg. The progenitor star of the SN has a 6-8 M He core with essentially no H envelope (< 5 × 10-4M) prior to the explosion. The main-sequence mass of the progenitor is estimated to be MMS = 20-25M, with additional systematic uncertainties due to convection, mass loss, rotation, and binary effects. These properties are intermediate between those of normal SNe and hypernovae associated with gamma-ray bursts. The mass of the central remnant is estimated as 1.6-1.8 M, which is near the boundary between neutron star and black hole formation.

本文言語English
ページ(範囲)1131-1142
ページ数12
ジャーナルAstrophysical Journal
692
2
DOI
出版ステータスPublished - 2009 2 20
外部発表はい

ASJC Scopus subject areas

  • 天文学と天体物理学
  • 宇宙惑星科学

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