Results 131 to 140 of about 249,735 (272)

A wind environment and Lorentz factors of tens explain gamma-ray bursts X-ray plateau. [PDF]

Nat Commun, 2022
Dereli-Bégué H, Pe'er A, Ryde F, Oates SR, Zhang B, Dainotti MG.   +5 more
europepmc   +1 more source

A Millimeter Rebrightening in GRB 210702A

The Astrophysical Journal
We present X-ray to radio frequency observations of the bright long gamma-ray burst GRB 210702A. Our Atacama Large Millimeter/submillimeter Array 97.5 GHz observations show a significant rebrightening by a factor of ≈2 beginning at 8.2 days post-burst ...
Simon de Wet, Tanmoy Laskar, Paul J. Groot, Rodolfo Barniol Duran, Edo Berger, Shivani Bhandari, Tarraneh Eftekhari, Cristiano Guidorzi, Shiho Kobayashi, Daniel A. Perley, Re’em Sari, Genevieve Schroeder   +11 more
doaj   +1 more source

Gamma ray bursts: A review of recent high-precision measurements [PDF]

Recent measurements and discoveries in gamma ray bursts and transients are reviewed including observations of the red shifted annihilation line in two kinds of slow transients (in 'classical' gamma ray bursts and in the unique 1979 March 5th event); of ...
Cline, T. L.
core   +1 more source

Correlation between Peak Energy and Peak Luminosity in Short Gamma-Ray Bursts

, 2012
A correlation between the peak luminosity and the peak energy has been found by Yonetoku et al. as $L_{p}\propto E_{p,i}^{2.0}$ for 11 pre-Swift long gamma-ray bursts. In this study, for a greatly expanded sample of 148 long gamma-ray bursts in the Swift
Chen, D. Y., Huang, Y. F., Zhang, Z. B.
core   +1 more source

A lanthanide-rich kilonova in the aftermath of a long gamma-ray burst [PDF]

, 2023
Yu-Han Yang, E. Troja, Brendan O’Connor, Chris L. Fryer, Myungshin Im, Joe Durbak, Gregory S. H. Paek, R. Ricci, C. R. Bom, J. H. Gillanders, A. J. Castro–Tirado, Zong-Kai Peng, S. Dichiara, Geoffrey Ryan, Hendrik van Eerten, Zi-Gao Dai, Seo-Won Chang, Hyeonho Choi, Kishalay De, Y. D. Hu, C. D. Kilpatrick, A. Kutyrev, Mankeun Jeong, Chung‐Uk Lee, Martı́n Makler, Felipe Navarete, Ignacio Pérez-García   +26 more
openalex   +1 more source

A Subclass of Gamma-Ray Burst Originating from Compact Binary Merger

The Astrophysical Journal
Type I gamma-ray bursts (GRBs) are believed to originate from compact binary mergers usually with a duration of main emission less than 2 s. However, recent observations of GRB 211211A and GRB 230307A indicate that some merger-origin GRBs could last much
Chen-Wei Wang, Wen-Jun Tan, Shao-Lin Xiong, Shu-Xu Yi, Rahim Moradi, Bing Li, Zhen Zhang, Yu Wang, Yan-Zhi Meng, Bo-Bing Wu, Jia-Cong Liu, Yue Wang, Sheng-Lun Xie, Wang-Chen Xue, Zheng-Hang Yu, Peng Zhang, Wen-Long Zhang, Yan-Qiu Zhang, Chao Zheng   +18 more
doaj   +1 more source

Gamma-ray burst variability above 4 MeV [PDF]

The relationship between the hard X-ray and gamma ray emissions during four bursts using the anti-coincidence shields of the High Energy Astronomy Observatory 3 (HEAO 3) Gamma Ray Spectrometer is explored.
Jacobson, A. S., Ling, J. C., Mahoney, W. A., Schwartz, R. A., Wheaton, W. A.   +4 more
core   +1 more source

Analysis of Gamma-Ray Burst Closure Relationship in Multiple Wavelengths

The Astrophysical Journal
Gamma-ray bursts (GRBs) are intense pulses of high-energy emission associated with the death of massive stars or compact objects’ coalescence. Their multiwavelength observations help verify the reliability of the standard fireball model.
M. G. Dainotti, S. Bhardwaj, E. Bissaldi, N. Fraija, S. Sourav, A. Galvan-Gamez   +5 more
doaj   +1 more source

The Afterglow, Energetics, and Host Galaxy of the Short‐Hard Gamma‐Ray Burst 051221a [PDF]

, 2006
A.M. Soderberg, E. Berger, M. Kasliwal, D. A. Frail, P. A. Price, Brian P. Schmidt, SR Kulkarni, D. B. Fox, S. B. Cenko, A. Gal-Yam, E. Nakar, Katherine C. Roth, A.M. Soderberg, E. Berger, M. Kasliwal, D. A. Frail, P. A. Price, Brian P. Schmidt, SR Kulkarni, D. B. Fox, S. B. Cenko, A. Gal-Yam, E. Nakar, Katherine C. Roth   +23 more
openalex   +1 more source

Contribution of γ-Ray Burst Afterglow Emissions to the Isotropic Diffuse γ-Ray Background

The Astrophysical Journal
The isotropic diffuse γ -ray background (IGRB) serves as a fundamental probe of the evolution of the extreme Universe. Although various astrophysical sources have been proposed as potential contributors to the IGRB, the dominant population is still under
Fang-Sheng Min, Yu-Hua Yao, Ruo-Yu Liu, Shi Chen, Hong Lu, Yi-Qing Guo   +5 more
doaj   +1 more source