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. 2017 Nov 2;551(7678):75-79.
doi: 10.1038/nature24303. Epub 2017 Oct 16.

A kilonova as the electromagnetic counterpart to a gravitational-wave source

S J Smartt  1 T-W Chen  2 A Jerkstrand  3 M Coughlin  4 E Kankare  1 S A Sim  1 M Fraser  5 C Inserra  6 K Maguire  1 K C Chambers  7 M E Huber  7 T Krühler  2 G Leloudas  8 M Magee  1 L J Shingles  1 K W Smith  1 D R Young  1 J Tonry  7 R Kotak  1 A Gal-Yam  9 J D Lyman  10 D S Homan  11 C Agliozzo  12   13 J P Anderson  14 C R Angus  6 C Ashall  15 C Barbarino  16 F E Bauer  13   17   18 M Berton  19   20 M T Botticella  21 M Bulla  22 J Bulger  7 G Cannizzaro  23   24 Z Cano  25 R Cartier  6 A Cikota  26 P Clark  1 A De Cia  26 M Della Valle  21   27 L Denneau  7 M Dennefeld  28 L Dessart  29 G Dimitriadis  6 N Elias-Rosa  30 R E Firth  6 H Flewelling  7 A Flörs  3   26   31 A Franckowiak  32 C Frohmaier  33 L Galbany  34 S González-Gaitán  35 J Greiner  2 M Gromadzki  36 A Nicuesa Guelbenzu  37 C P Gutiérrez  6 A Hamanowicz  26   36 L Hanlon  5 J Harmanen  38 K E Heintz  8   39 A Heinze  7 M-S Hernandez  40 S T Hodgkin  41 I M Hook  42 L Izzo  25 P A James  15 P G Jonker  23   24 W E Kerzendorf  26 S Klose  37 Z Kostrzewa-Rutkowska  23   24 M Kowalski  32   43 M Kromer  44   45 H Kuncarayakti  38   46 A Lawrence  11 T B Lowe  7 E A Magnier  7 I Manulis  9 A Martin-Carrillo  5 S Mattila  38 O McBrien  1 A Müller  47 J Nordin  43 D O'Neill  1 F Onori  23   24 J T Palmerio  48 A Pastorello  49 F Patat  26 G Pignata  12   13 Ph Podsiadlowski  50 M L Pumo  49   51   52 S J Prentice  15 A Rau  2 A Razza  14   53 A Rest  54   55 T Reynolds  38 R Roy  16   56 A J Ruiter  57   58   59 K A Rybicki  36 L Salmon  5 P Schady  2 A S B Schultz  7 T Schweyer  2 I R Seitenzahl  57   58 M Smith  6 J Sollerman  16 B Stalder  60 C W Stubbs  61 M Sullivan  6 H Szegedi  62 F Taddia  16 S Taubenberger  3   26 G Terreran  49   63 B van Soelen  62 J Vos  40 R J Wainscoat  7 N A Walton  41 C Waters  7 H Weiland  7 M Willman  7 P Wiseman  2 D E Wright  64 Ł Wyrzykowski  36 O Yaron  9
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A kilonova as the electromagnetic counterpart to a gravitational-wave source

S J Smartt et al. Nature. .

Abstract

Gravitational waves were discovered with the detection of binary black-hole mergers and they should also be detectable from lower-mass neutron-star mergers. These are predicted to eject material rich in heavy radioactive isotopes that can power an electromagnetic signal. This signal is luminous at optical and infrared wavelengths and is called a kilonova. The gravitational-wave source GW170817 arose from a binary neutron-star merger in the nearby Universe with a relatively well confined sky position and distance estimate. Here we report observations and physical modelling of a rapidly fading electromagnetic transient in the galaxy NGC 4993, which is spatially coincident with GW170817 and with a weak, short γ-ray burst. The transient has physical parameters that broadly match the theoretical predictions of blue kilonovae from neutron-star mergers. The emitted electromagnetic radiation can be explained with an ejected mass of 0.04 ± 0.01 solar masses, with an opacity of less than 0.5 square centimetres per gram, at a velocity of 0.2 ± 0.1 times light speed. The power source is constrained to have a power-law slope of -1.2 ± 0.3, consistent with radioactive powering from r-process nuclides. (The r-process is a series of neutron capture reactions that synthesise many of the elements heavier than iron.) We identify line features in the spectra that are consistent with light r-process elements (atomic masses of 90-140). As it fades, the transient rapidly becomes red, and a higher-opacity, lanthanide-rich ejecta component may contribute to the emission. This indicates that neutron-star mergers produce gravitational waves and radioactively powered kilonovae, and are a nucleosynthetic source of the r-process elements.

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