Optical superluminal motion measurement in the neutron-star merger GW170817

Kunal P Mooley; Jay Anderson; Wenbin Lu

doi:10.1038/s41586-022-05145-7

Optical superluminal motion measurement in the neutron-star merger GW170817

Nature. 2022 Oct;610(7931):273-276. doi: 10.1038/s41586-022-05145-7. Epub 2022 Oct 12.

Authors

Kunal P Mooley^#^{1

2}, Jay Anderson^#³, Wenbin Lu^#^{4

5

6

7}

Affiliations

¹ Caltech, Pasadena, CA, USA. kunal@astro.caltech.edu.
² National Radio Astronomy Observatory, Socorro, NM, USA. kunal@astro.caltech.edu.
³ Space Telescope Science Institute, Baltimore, MD, USA. jayander@stsci.edu.
⁴ Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA.
⁵ Department of Astronomy, UC Berkeley, Berkeley, CA, USA.
⁶ Theoretical Astrophysics Center, UC Berkeley, Berkeley, CA, USA.
⁷ TAPIR, Walter Burke Institute for Theoretical Physics, Caltech, Pasadena, CA, USA.

^# Contributed equally.

PMID: 36224419
DOI: 10.1038/s41586-022-05145-7

Abstract

The afterglow of the binary neutron-star merger GW170817¹ gave evidence for a structured relativistic jet^2-6 and a link^3,7,8 between such mergers and short gamma-ray bursts. Superluminal motion, found using radio very long baseline interferometry³ (VLBI), together with the afterglow light curve provided constraints on the viewing angle (14-28 degrees), the opening angle of the jet core (less than 5 degrees) and a modest limit on the initial Lorentz factor of the jet core (more than 4). Here we report on another superluminal motion measurement, at seven times the speed of light, leveraging Hubble Space Telescope precision astrometry and previous radio VLBI data for GW170817. We thereby obtain a measurement of the Lorentz factor of the wing of the structured jet, as well as substantially improved constraints on the viewing angle (19-25 degrees) and the initial Lorentz factor of the jet core (more than 40).

Publication types

Research Support, Non-U.S. Gov't
Research Support, U.S. Gov't, Non-P.H.S.