GRB 170817A Associated with GW170817: Multi-frequency Observations and Modeling of Prompt Gamma-Ray Emission

作者：Pozanenko A S^*; Barkov M V; Minaev P Yu; Volnova A A; Mazaeva E D; Moskvitin A S; Krugov M A; Samodurov V A; Loznikov V M; Lyutikov M

来源：Astrophysical Journal Letters, 2018, 852(2): L30.

DOI：10.3847/2041-8213/aaa2f6

• accretion, accretion disks
• gamma-ray burst: individual (GRB 170817A)
• gravitational waves
• radio continuum: general
• techniques: photometric

We present our observations of electromagnetic transients associated with GW170817/GRB. 170817A using optical telescopes of Chilescope observatory and Big Scanning Antenna (BSA) of Pushchino Radio Astronomy Observatory at 110. MHz. The Chilescope observatory detected an optical transient of similar to 19(m) on the third day in the outskirts of the galaxy NGC 4993; we continued observations following its rapid decrease. We put an upper limit of 1.5 x 10(4) Jy on any radio source with a duration of 10-60 s, which may be associated with GW170817/ GRB. 170817A. The prompt gamma-ray emission consists of two distinctive components-a hard short pulse delayed by similar to 2 s with respect to the LIGO signal and softer thermal pulse with T similar to 10 keV lasting for another similar to 2 s. The appearance of a thermal component at the end of the burst is unusual for short GRBs. Both the hard and the soft components do not satisfy the Amati relation, making GRB. 170817A distinctively different from other short GRBs. Based on gamma-ray and optical observations, we develop a model for the prompt high-energy emission associated with GRB. 170817A. The merger of two neutron stars creates an accretion torus of similar to 10(-2) Me, which supplies the black hole with magnetic flux and confines the Blandford-Znajek-powered jet. We associate the hard prompt spike with the quasispherical breakout of the jet from the disk wind. As the jet plows through the wind with subrelativistic velocity, it creates a radiation-dominated shock that heats the wind material to tens of kiloelectron volts, producing the soft thermal component.

• 出版日期2018-1-10