The Afterglow and Kilonova of the Short GRB 160821B

التفاصيل البيبلوغرافية
العنوان: The Afterglow and Kilonova of the Short GRB 160821B
المؤلفون: E. Troja, A. J. Castro-Tirado, J Becerra Gonzalez, Y. Hu, G. S. Ryan, S. B. Cenko, R. Ricci, G. Novara, R. Sanchez-Ramirez, J. A. Acosta-Pulido, K. D. Ackley, M. D. Caballero Garcıa, S. S. Eikenberry, S. Guziy, S. Jeong, A. Y. Lien, I. Marquez, S. B. Pandey, I. H. Park, T. Sakamoto, J. C. Tello, I. V. Sokolov, V. V. Sokolov, A. Tiengo, A. F. Valeev, B. B. Zhang, S. Veilleux
المصدر: Monthly Notices of the Royal Astronomical Society. 489(2)
بيانات النشر: United States: NASA Center for Aerospace Information (CASI), 2019.
سنة النشر: 2019
مصطلحات موضوعية: Astronomy
الوصف: GRB 160821B is a short duration gamma-ray burst (GRB) detected and localized by the Neil Gehrels Swift Observatory in the outskirts of a spiral galaxy at z = 0.1613, at a projected physical offset of 16 kpc from the galaxy’s center. We present X-ray, optical/nIR, and radio observations of its counterpart and model them with two distinct components of emission: a standard afterglow, arising from the interaction of the relativistic jet with the surrounding medium, and a kilonova, powered by the radioactive decay of the sub-relativistic ejecta. Broadband modelling of the afterglow data reveals a weak reverse shock propagating backward into the jet, and a likely jet-break at 3.5 d. This is consistent with a structured jet seen slightly off-axis (θview ∼ θcore) while expanding into a low-density medium (n ≈ 10−3 cm−3). Analysis of the kilonova properties suggests a rapid evolution towards red colours, similar toAT2017gfo, and a low-nIR luminosity, possibly due to the presence of a long-lived neutron star. The global properties of the environment, the inferred low mass (Mej <~ 0.006 Msun) and velocities (vej >~ 0.05c) of lanthanide-rich ejecta are consistent with a binary neutron star merger progenitor.
نوع الوثيقة: Report
اللغة: English
تدمد: 1365-2966
0035-8711
DOI: 10.1093/mnras/stz2255
URL الوصول: https://ntrs.nasa.gov/citations/20210014088
ملاحظات: 80GSFC17M0002

789737

NSF AST-1005313

STSI HST-GO14357

STSI HST-GO14087

STSI HST-GO14607

STSI HST-GO14850

SEV-2017-0709

AST-0352664

2015-046-R.0

EUH 654215

201406660015

ASI–INAF 2017-14-H.0
رقم الانضمام: edsnas.20210014088
قاعدة البيانات: NASA Technical Reports
الوصف
تدمد:13652966
00358711
DOI:10.1093/mnras/stz2255