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

Daryl Haggard, Melania Nynka, John J. Ruan, Vicky Kalogera, S. Bradley Cenko, Phil Evans, Jamie A. Kennea

Research output: Contribution to journalArticle

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Abstract

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 (Δt ∼ 2 days) and Swift (Δt ∼ 1-3 days) observations yielded non-detections 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 (Δt ∼ 15-16 days). We detect X-ray emission from SSS17a with L0.3-10 keV = 2.6+0.5-0.4 × 1038erg 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 (L0.3-10 keV ∼9 ×1038 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.

Original languageEnglish (US)
Article numberL25
JournalAstrophysical Journal Letters
Volume848
Issue number2
DOIs
StatePublished - Oct 20 2017

Fingerprint

coalescence
coalescing
neutron stars
LIGO (observatory)
gravitational waves
point sources
point source
bursts
rays
x rays
electromagnetism
afterglows
erg
merger
line of sight
light curve
power law
actuators
galaxies
monitoring

Keywords

  • X-rays: binaries
  • galaxies: individual (NGC 4993)
  • gamma-ray burst: individual (GRB 170817A)
  • gravitational waves
  • stars: neutron

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Haggard, D., Nynka, M., Ruan, J. J., Kalogera, V., Cenko, S. B., Evans, P., & Kennea, J. A. (2017). A Deep Chandra X-Ray Study of Neutron Star Coalescence GW170817. Astrophysical Journal Letters, 848(2), [L25]. https://doi.org/10.3847/2041-8213/aa8ede
Haggard, Daryl ; Nynka, Melania ; Ruan, John J. ; Kalogera, Vicky ; Cenko, S. Bradley ; Evans, Phil ; Kennea, Jamie A. / A Deep Chandra X-Ray Study of Neutron Star Coalescence GW170817. In: Astrophysical Journal Letters. 2017 ; Vol. 848, No. 2.
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Haggard, D, Nynka, M, Ruan, JJ, Kalogera, V, Cenko, SB, Evans, P & Kennea, JA 2017, 'A Deep Chandra X-Ray Study of Neutron Star Coalescence GW170817', Astrophysical Journal Letters, vol. 848, no. 2, L25. https://doi.org/10.3847/2041-8213/aa8ede

A Deep Chandra X-Ray Study of Neutron Star Coalescence GW170817. / Haggard, Daryl; Nynka, Melania; Ruan, John J.; Kalogera, Vicky; Cenko, S. Bradley; Evans, Phil; Kennea, Jamie A.

In: Astrophysical Journal Letters, Vol. 848, No. 2, L25, 20.10.2017.

Research output: Contribution to journalArticle

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T1 - A Deep Chandra X-Ray Study of Neutron Star Coalescence GW170817

AU - Haggard, Daryl

AU - Nynka, Melania

AU - Ruan, John J.

AU - Kalogera, Vicky

AU - Cenko, S. Bradley

AU - Evans, Phil

AU - Kennea, Jamie A.

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N2 - 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 (Δt ∼ 2 days) and Swift (Δt ∼ 1-3 days) observations yielded non-detections 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 (Δt ∼ 15-16 days). We detect X-ray emission from SSS17a with L0.3-10 keV = 2.6+0.5-0.4 × 1038erg 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 (L0.3-10 keV ∼9 ×1038 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.

AB - 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 (Δt ∼ 2 days) and Swift (Δt ∼ 1-3 days) observations yielded non-detections 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 (Δt ∼ 15-16 days). We detect X-ray emission from SSS17a with L0.3-10 keV = 2.6+0.5-0.4 × 1038erg 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 (L0.3-10 keV ∼9 ×1038 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.

KW - X-rays: binaries

KW - galaxies: individual (NGC 4993)

KW - gamma-ray burst: individual (GRB 170817A)

KW - gravitational waves

KW - stars: neutron

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