A Deep Chandra X-Ray Study of Neutron Star Coalescence GW170817

摘要

We report Chandra observations of GW170817, the first neutron star-neutron star merger discovered by the joint LIGO-Virgo Collaboration, and the first direct detection of gravitational radiation associated with an electromagnetic counterpart, Fermi short γ-ray burst GRB 170817A. The event occurred on 2017 August 17 and subsequent observations identified an optical counterpart, SSS17a, coincident with NGC 4993 (～10" separation). Early Chandra (△t ~ 2 days) and Swift (△t ~ 1-3 days) observations yielded nondetections at the optical position, but ～9 days post-trigger Chandra monitoring revealed an X-ray point source coincident with SSS17a. We present two deep Chandra observations totaling ～95 ks, collected on 2017 September 01-02 (△t ~ 15-16 days). We detect X-ray emission from SSS17a with L_(0.3-10 keV)=2.6~(+0.5)_(0.4)×10~(38) erg s~(-1), and a power law spectrum of Γ = 2.4 ± 0.8. We find that the X-ray light curve from a binary NS coalescence associated with this source is consistent with the afterglow from an off-axis short γ-ray burst, with a jet angled ? 23° from the line of sight. This event marks both the first electromagnetic counterpart to a LIGO-Virgo gravitational-wave source and the first identification of an off-axis short GRB. We also confirm extended X-ray emission from NGC 4993 (L_(0.3-10 keV) ~ 9 × 10~(38) erg s~(-1)) consistent with its E/S0 galaxy classification, and report two new Chandra point sources in this field, CXOU J130948 and CXOU J130946.