TY - JOUR
T1 - GRB 250704B
T2 - An Off-axis Short GRB with a Long-lived Afterglow Plateau
AU - Swain, Vishwajeet
AU - Ahumada, Tomás
AU - Patil, Sameer K.
AU - Wagh, Yogesh
AU - Bhalerao, Varun
AU - Nakar, Ehud
AU - Kasliwal, Mansi
AU - Hall, Xander J.
AU - Busmann, Malte
AU - Pathak, Utkarsh
AU - Anand, Shreya
AU - Karambelkar, Viraj
AU - Andreoni, Igor
AU - Anupama, G. C.
AU - Arya, Anuraag
AU - Balasubramanian, Arvind
AU - Barway, Sudhanshu
AU - Carney, Jonathan
AU - Coughlin, Michael
AU - Eappachen, D.
AU - Freeburn, James
AU - Gruen, Daniel
AU - Mohan, Tanishk
AU - O’Connor, Brendan
AU - Palmese, Antonella
AU - Sahu, D. K.
AU - Saikia, Aditya Pawan
AU - Sarin, Nikhil
AU - Srinivasaragavan, Gokul
AU - Tanenia, Hitesh
N1 - Publisher Copyright:
© 2026. The Author(s). Published by the American Astronomical Society.
PY - 2026/1/10
Y1 - 2026/1/10
N2 - We present a detailed multiwavelength afterglow study of the short gamma-ray burst (GRB) GRB 250704B, extensively monitored in optical and near-infrared bands. Its afterglow displays an unusually long duration plateau followed by an achromatic break and a steep decline, deviating from canonical GRB afterglows. While long plateaus are often explained by central engine activity, we find that for GRB 250704B an energy injection model requires unreasonable parameters. The afterglow is better explained by an off-axis power-law structured jet with a narrow core (θc ≈ 0. °7) viewed at a modest angle (θv ≈ 1. °9). A comparison with GRB 170817A shows that both events are consistent with the off-axis structured jet scenario, where the shape of the light curve is governed primarily by the geometry of the jet and the viewing angle rather than the energetics, microphysical parameters, or external density. Our results underscore the importance of incorporating the jet structure in GRB modeling.
AB - We present a detailed multiwavelength afterglow study of the short gamma-ray burst (GRB) GRB 250704B, extensively monitored in optical and near-infrared bands. Its afterglow displays an unusually long duration plateau followed by an achromatic break and a steep decline, deviating from canonical GRB afterglows. While long plateaus are often explained by central engine activity, we find that for GRB 250704B an energy injection model requires unreasonable parameters. The afterglow is better explained by an off-axis power-law structured jet with a narrow core (θc ≈ 0. °7) viewed at a modest angle (θv ≈ 1. °9). A comparison with GRB 170817A shows that both events are consistent with the off-axis structured jet scenario, where the shape of the light curve is governed primarily by the geometry of the jet and the viewing angle rather than the energetics, microphysical parameters, or external density. Our results underscore the importance of incorporating the jet structure in GRB modeling.
UR - https://www.scopus.com/pages/publications/105033493157
UR - https://www.scopus.com/pages/publications/105033493157#tab=citedBy
U2 - 10.3847/2041-8213/ae2a20
DO - 10.3847/2041-8213/ae2a20
M3 - Article
AN - SCOPUS:105033493157
SN - 2041-8205
VL - 996
JO - Astrophysical Journal Letters
JF - Astrophysical Journal Letters
IS - 2
M1 - L38
ER -