AN ACHROMATIC BREAK IN THE AFTERGLOW OF THE SHORT GRB 140903A: EVIDENCE FOR A NARROW JET

作者：Troja E; Sakamoto T; Cenko S B; Lien A; Gehrels N; Castro Tirado A J; Ricci R; Capone J; Toy V; Kutyrev A; Kawai N; Cucchiara A; Fruchter A; Gorosabel J; Jeong S; Levan A; Perley D; Sanchez Ramirez R; Tanvir N; Veilleux S

来源：Astrophysical Journal, 2016, 827(2): 102.

DOI：10.3847/0004-637X/827/2/102

• gamma-ray burst: individual (GRB 140903A)
• X-rays: bursts

We report the results of our observing campaign on GRB. 140903A, a nearby (z = 0.351) short-duration (T-90 similar to 0.3 s) gamma-ray burst discovered by Swift. We monitored the X-ray afterglow with Chandra up to 15 days after the burst. and detected a steeper decay of the X-ray flux after t(j) approximate to 1 day. Continued monitoring at optical and radio wavelengths showed a similar decay in flux at nearly the same time, and we interpret it as evidence of a narrowly collimated jet. By using the standard fireball model to describe the afterglow evolution, we derive a jet opening angle theta(j) approximate to 5 degrees and a collimation-corrected total energy release E approximate to 2 x 10(50) erg. We further discuss the nature of the GRB progenitor system. Three main lines disfavor a massive star progenitor: the properties of the prompt gamma-ray emission, the age and low star formation rate of the host galaxy, and the lack of a bright supernova. We conclude that this event. likely originated from a compact binary merger.

• 出版日期2016-8-20