The unpolarized macronova associated with the gravitational wave event GW 170817

S. Covino, K. Wiersema, Y. Z. Fan, K. Toma, A. B. Higgins, A. Melandri, P. D'Avanzo, C. G. Mundell, E. Palazzi, N. R. Tanvir, M. G. Bernardini, M. Branchesi, E. Brocato, S. Campana, S. Di Serego Alighieri, D. Götz, J. P.U. Fynbo, W. Gao, A. Gomboc, B. GompertzJ. Greiner, J. Hjorth, Z. P. Jin, L. Kaper, S. Klose, S. Kobayashi, D. Kopac, C. Kouveliotou, A. J. Levan, J. Mao, D. Malesani, E. Pian, A. Rossi, R. Salvaterra, R. L.C. Starling, I. Steele, G. Tagliaferri, E. Troja, A. J. Van Der Horst, R. A.M.J. Wijers

Research output: Contribution to journalArticlepeer-review

66 Citations (Scopus)


The merger of two dense stellar remnants including at least one neutron star is predicted to produce gravitational waves (GWs) and short-duration gamma ray bursts 1,2. In the process, neutron-rich material is ejected from the system and heavy elements are synthesized by r-process nucleosynthesis 1,3. The radioactive decay of these heavy elements produces additional transient radiation termed kilonova or macronova 4-10. We report the detection of linear optical polarization, P = (0.50 ± 0.07)%, 1.46 days after detection of the GWs from GW 170817-a double neutron star merger associated with an optical macronova counterpart and a short gamma ray burst 11-14. The optical emission from a macronova is expected to be characterized by a blue, rapidly decaying component and a red, more slowly evolving component due to material rich in heavy elements-the lanthanides 15. The polarization measurement was made when the macronova was still in its blue phase, during which there was an important contribution from a lanthanide-free outflow. The low degree of polarization is consistent with intrinsically unpolarized emission scattered by galactic dust, suggesting a symmetric geometry of the emitting region and low inclination of the merger system. Stringent upper limits to the polarization degree from 2.45-9.48 days post-burst are consistent with the lanthanides-rich macronova interpretation.

Original languageEnglish
Pages (from-to)791-794
Number of pages4
JournalNature Astronomy
Issue number11
Publication statusPublished - 2017 Nov 1

ASJC Scopus subject areas

  • Astronomy and Astrophysics


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