Evidence for X-Ray emission in excess to the jet-afterglow decay 3.5 yr after the binary neutron star merger GW 170817: a new emission component
A. Hajela, R. Margutti, J.S. Bright, K.D. Alexander, B.D. Metzger, V. Nedora, A. Kathirgamaraju, B. Margalit, D. Radice, E. Berger, A. MacFadyen, D. Giannios, R. Chornock, I. Heywood, L. Sironi, O. Gottlieb, D. Coppejans, T. Laskar, Y. Cendes, R.B. DuranT. Eftekhari, W. Fong, A. McDowell, M. Nicholl, X. Xie, J. Zrake, S. Bernuzzi, F.S. Broekgaarden, C.D. Kilpatrick, G. Terreran, V.A. Villar, P.K. Blanchard, S. Gomez, G. Hosseinzadeh, D.J. Matthews, J.C. Rastinejad
Research output: Contribution to journal › Article › peer-review
118Downloads
(Pure)
Fingerprint
Dive into the research topics of 'Evidence for X-Ray emission in excess to the jet-afterglow decay 3.5 yr after the binary neutron star merger GW 170817: a new emission component'. Together they form a unique fingerprint.