2019Sci...363..968G

Query : 2019Sci...363..968G

2019Sci...363..968G - Science, 363, 968-971 (2019)

Compact radio emission indicates a structured jet was produced by a binary neutron star merger.

GHIRLANDA G., SALAFIA O.S., PARAGI Z., GIROLETTI M., YANG J., MARCOTE B., BLANCHARD J., AGUDO I., AN T., BERNARDINI M.G., BESWICK R., BRANCHESI M., CAMPANA S., CASADIO C., CHASSANDE-MOTTIN E., COLPI M., COVINO S., D'AVANZO P., D'ELIA V., FREY S., GAWRONSKI M., GHISELLINI G., GURVITS L.I., JONKER P.G., VAN LANGEVELDE H.J., MELANDRI A., MOLDON J., NAVA L., PEREGO A., PEREZ-TORRES M.A., REYNOLDS C., SALVATERRA R., TAGLIAFERRI G., VENTURI T., VERGANI S.D. and ZHANG M.

Journal keyword(s):

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 Fermi bn170817908 gB 05 32 +50.1           ~ 30 0
2 NGC 4993 Sy2 13 09 47.6908761600 -23 23 02.314044636   13.34   11.92   ~ 397 0
3 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2683 0

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