SIMBAD references

2007A&A...465L..29C - Astronomy and Astrophysics, volume 465, L29-33 (2007/4-2)

Binary star progenitors of long gamma-ray bursts.

CANTIELLO M., YOON S.-C., LANGER N. and LIVIO M.

Abstract (from CDS):

The collapsar model for long gamma-ray bursts requires a rapidly rotating Wolf-Rayet star as progenitor. We test the idea of producing rapidly rotating Wolf-Rayet stars in massive close binaries through mass accretion and consecutive quasi-chemically homogeneous evolution - the latter had previously been shown to provide collapsars below a certain metallicity threshold. We use a 1D hydrodynamic binary evolution code to simulate the evolution of a 16+15M binary model with an initial orbital period of 5 days and SMC metallicity (Z=0.004). Internal differential rotation, rotationally induced mixing and magnetic fields are included in both components, as well as non-conservative mass and angular momentum transfer, and tidal spin-orbit coupling. The considered binary system undergoes early Case B mass transfer. The mass donor becomes a helium star and dies as a type Ib/c supernova. The mass gainer is spun-up, and internal magnetic fields efficiently transport accreted angular momentum into the stellar core. The orbital widening prevents subsequent tidal synchronization, and the mass gainer rejuvenates and evolves quasi-chemically homogeneously thereafter. The mass donor explodes 7Myr before the collapse of the mass gainer. Assuming the binary to be broken-up by the supernova kick, the potential gamma-ray burst progenitor would become a runaway star with a space velocity of 27km/s, traveling about 200pc during its remaining lifetime. The binary channel presented here does not, as such, provide a new physical model for collapsar production, as the resulting stellar models are almost identical to quasi-chemically homogeneously evolving rapidly rotating single stars. However, it may provide a means for massive stars to obtain the required high rotation rates. Moreover, it suggests that a possibly large fraction of long gamma-ray bursts occurs in runaway stars.

Abstract Copyright:

Journal keyword(s): stars: binaries: general - stars: rotation - stars: evolution - stars: mass-loss - supernovae: general - gamma rays: bursts

Simbad objects: 2

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2020.01.26-00:28:26

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