The diverse lives of progenitors of hydrogen-rich core-collapse supernovae: the role of binary interaction

@article{Zapartas2019TheDL,
  title={The diverse lives of progenitors of hydrogen-rich core-collapse supernovae: the role of binary interaction},
  author={Emmanouil Zapartas and Selma E. de Mink and Stephen Justham and Nathan Smith and Alexander de Koter and Mathieu Renzo and Iair Arcavi and Robert Farmer and Ylva G{\"o}tberg and Silvia Toonen},
  journal={Astronomy \& Astrophysics},
  year={2019}
}
Hydrogen-rich supernovae, known as Type II (SNe II), are the most common class of explosions observed following the collapse of the core of massive stars. We used analytical estimates and population synthesis simulations to assess the fraction of SNe II progenitors that are expected to have exchanged mass with a companion prior to explosion. We estimate that 1/3 to 1/2 of SN II progenitors have a history of mass exchange with a binary companion before exploding. The dominant binary channels… Expand

Figures and Tables from this paper

The explosive life of massive binaries
Massive stars are born predominantly as members of binary (or higher multiplicity) systems, and the presence of a companion can significantly alter their life and final fate. Therefore, any observedExpand
Observability of inflated companion stars after supernovae in massive binaries
We carry out a systematic study of the response of companion stars in massive binaries after being impacted by supernova ejecta. A total of 720 1D stellar evolution calculations are performed toExpand
The 50–100 pc scale parent stellar populations of Type II supernovae and limitations of single star evolution models
There is observational evidence of a dearth in core-collapse supernova (ccSN) explosions from stars with zero-age main-sequence (ZAMS) mass M0 ≈ 17–30M⊙, referred to as the ‘red supergiantExpand
The Explosion Mechanism of Core-Collapse Supernovae and Its Observational Signatures
The death of massive stars is shrouded in many mysteries. One of them is the mechanism that overturns the collapse of the degenerate iron core into an explosion, a process that determines theExpand
Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants
The diversity of Type II supernovae (SNe II) is thought to be driven mainly by differences in their progenitor’s hydrogen-rich (H-rich) envelope mass, with SNe IIP having long plateaus (∼100 days)Expand
Live fast and die young : Evolution and fate of massive stars
This thesis investigates several aspects of the evolution of massive stars and binaries, with particular attention to the final fate of the star, and the implications of the stellar death forExpand
Long-term evolution of a magnetic massive merger product
About 10% of stars more massive than ${\approx}\,1.5\,\mathrm{M}_\odot$ have strong, large-scale surface magnetic fields and are being discussed as progenitors of highly-magnetic white dwarfs andExpand
The origins of low-luminosity supernovae: the case of SN 2016bkv
We investigate the low-luminosity supernova SN 2016bkv and its peculiar early-time interaction. For that, we compute radiative transfer models using the cmfgen code. Because SN 2016bkv shows signsExpand
The uncertain masses of progenitors of core-collapse supernovae and direct-collapse black holes
We show that it is not possible to determine the final mass $M_{\rm fin}$ of a red supergiant (RSG) at the pre-supernova (SN) stage from its luminosity $L$ and effective temperature $T_{\rm eff}$Expand
The Red Supergiant Binary Fraction of the Large Magellanic Cloud
The binary fraction of unevolved massive stars is thought to be 70-100% but there are few observational constraints on the binary fraction of the evolved version of a subset of these stars, the redExpand
...
1
2
3
...

References

SHOWING 1-10 OF 181 REFERENCES
Observed Fractions of Core-Collapse Supernova Types and Initial Masses of their Single and Binary Progenitor Stars
We analyse the observed fractions of core-collapse supernova (SN) types from the Lick Observatory Supernova Search (LOSS), and we discuss the corresponding implications for massive star evolution.Expand
Binary progenitor models of type IIb supernovae
Massive stars that lose their hydrogen-rich envelope down to a few tenths of a solar mass explode as extended type IIb supernovae, an intriguing subtype that links the hydrogen-rich type IIExpand
Delay-time distribution of core-collapse supernovae with late events resulting from binary interaction
Most massive stars, the progenitors of core-collapse supernovae, are in close binary systems and may interact with their companion through mass transfer or merging. We undertake a populationExpand
Progenitors of supernova Ibc: a single Wolf-Rayet star as the possible progenitor of the SN Ib iPTF13bvn
Core-collapse supernova (SN) explosions mark the end of the tumultuous life of massive stars. Determining the nature of their progenitors is a crucial step towards understanding the properties ofExpand
Predicting the Presence of Companions for Stripped-envelope Supernovae: The Case of the Broad-lined Type Ic SN 2002ap
Many young, massive stars are found in close binaries. Using population synthesis simulations we predict the likelihood of a companion star being present when these massive stars end their lives asExpand
TYPE Ib/c SUPERNOVAE IN BINARY SYSTEMS. I. EVOLUTION AND PROPERTIES OF THE PROGENITOR STARS
We investigate the evolution of Type Ib/c supernova (SN Ib/c) progenitors in close binary systems, using new evolutionary models that include the effects of rotation, with initial masses of 12-25 M ☉Expand
Measurement of the core-collapse progenitor mass distribution of the Small Magellanic Cloud
The physics of core-collapse (CC) supernovae (SNe) and how the explosions depend on progenitor properties are central questions in astronomy. For only a handful of SNe, the progenitor star has beenExpand
The death of massive stars - II. Observational constraints on the progenitors of type Ibc supernovae
The progenitors of many Type II core-collapse supernovae (SNe) have now been identified directly on pre-discovery imaging. Here, we present an extensive search for the progenitors of Type Ibc SNe inExpand
Constraints on core-collapse supernova progenitors from explosion site integral field spectroscopy
Observationally, supernovae (SNe) are divided into subclasses pertaining to their distinct characteristics. This diversity reflects the diversity in the progenitor stars. It is not entirely clear howExpand
The death of massive stars – I. Observational constraints on the progenitors of Type II-P supernovae
The progenitors of many type II core-collapse supernovae have now been identified directly on pre-discovery imaging. Here we present an extensive search for the progenitors of type Ibc supernovae inExpand
...
1
2
3
4
5
...