Progenitors of Core-Collapse Supernovae

@article{Smartt2009ProgenitorsOC,
  title={Progenitors of Core-Collapse Supernovae},
  author={Steven J. Smartt},
  journal={Annual Review of Astronomy and Astrophysics},
  year={2009},
  volume={47},
  pages={63-106}
}
  • S. Smartt
  • Published 5 August 2009
  • Physics
  • Annual Review of Astronomy and Astrophysics
Knowledge of the progenitors of core-collapse supernovae is a fundamental component in understanding the explosions. The recent progress in finding such stars is reviewed. The minimum initial mass that can produce a supernova (SN) has converged to 8 ± 1 M⊙ from direct detections of red supergiant progenitors of II-P SNe and the most massive white dwarf progenitors, although this value is model dependent. It appears that most type Ibc SNe arise from moderate mass interacting binaries. The highly… 
Progenitor constraints for core-collapse supernovae from Chandra X-ray observations
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  • J. Groh
  • Physics
    Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences
  • 2017
TLDR
Recent efforts to predict the nature of stars before death by performing coupled stellar evolution and atmosphere modelling of single stars in the pre-SN stage are reviewed, and the detectability of SN Ibc progenitors is assessed.
Observational Constraints on the Progenitors of Core-Collapse Supernovae: The Case for Missing High-Mass Stars
  • S. Smartt
  • Physics
    Publications of the Astronomical Society of Australia
  • 2015
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References

SHOWING 1-10 OF 305 REFERENCES
A giant outburst two years before the core-collapse of a massive star
TLDR
It is reported that the peculiar type Ib supernova SN 2006jc is spatially coincident with a bright optical transient that occurred in 2004, andSpectroscopic and photometric monitoring of the supernova leads us to suggest that the progenitor was a carbon-oxygen Wolf–Rayet star embedded within a helium-rich circumstellar medium.
The Nature of the Progenitor of the Type II-P Supernova 1999em*
The masses and the evolutionary states of the progenitors of core-collapse supernovae (SNe) are not well constrained by direct observations. Stellar evolution theory generally predicts that massive
The massive binary companion star to the progenitor of supernova 1993J
TLDR
Photometric and spectroscopic observations of SN1993J ten years after the explosion detect the unambiguous signature of a massive star: the binary companion to the progenitor.
Peculiar, low-luminosity Type II supernovae: low-energy explosions in massive progenitors?
A number of supernovae, classified as Type II, show remarkably peculiar properties such as an extremely low expansion velocity and an extraordinarily small amount of 5 6 Ni in the ejecta. We present
A massive hypergiant star as the progenitor of the supernova SN 2005gl
TLDR
It is reported that the previously proposed object was indeed the progenitor star of SN 2005gl, likely a luminous blue variable that standard stellar evolution predicts should not have exploded in that state.
How Much 56Ni Can Be Produced in Core-Collapse Supernovae? Evolution and Explosions of 30-100 M☉ Stars
Motivated by the discovery of extremely bright supernovae SNe 1999as and 2006gy, we have investigated how much 56Ni mass can be synthesized in core-collapse massive supernovae (SNe). We calculate the
Supernova Shock Breakout from a Red Supergiant
TLDR
Observations of the supernova SNLS-04D2dc with the Galaxy Evolution Explorer space telescope reveal a radiative precursor from thesupernova shock before the shock reached the surface of the star and show the initial expansion of thestar at the beginning of the explosion.
On the role of continuum-driven eruptions in the evolution of very massive stars and Population III stars
We suggest that the mass lost during the evolution of very massive stars may be dominated by optically thick, continuum-driven outbursts or explosions, instead of by steady line-driven winds. In
A non-spherical core in the explosion of supernova SN 2004dj
TLDR
Multi-epoch spectropolarimetry of a classic type II-P supernova reveals the abrupt appearance of significant polarization when the inner core is first exposed in the thinning ejecta (∼90 days after explosion), suggesting that a strongly non-spherical explosion may be a generic feature of core-collapse supernovae of all types.
Constraints on core-collapse supernova progenitors from correlations with Hα emission
We present observational constraints on the nature of the different core-collapse supernova (SN) types through an investigation of the association of their explosion sites with recent star formation
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