2017/10/31 by Chuan Yue, Qian Hu, Fu-Wen Zhang +5 · 1 citation
Immunology and Microbiology · Physics and Astronomy · #Afterglow #Alexander von Humboldt Studies #Astronomy and Astrophysical Research #Black hole (networking) #Gamma-ray burst #Gamma-ray bursts and supernovae #Neutron star #Redshift #astro-ph.HE #gr-qc
paper · pdf · doi:10.3847/2041-8213/aaa66c
published as The Astrophysical Journal Letters, 2018, Volume 853, Number 1 · 6 pages, 5 figures, published in ApJL 853 L10
openalex publication_date 2018/01/19 · arxiv created 2018/02/01 · arxiv updated 2018/02/02 · openalex created_date 2018/02/23 · openalex updated_date 2026/08/05
Abstract GRB 170817A is the first short gamma-ray burst (GRB) with direct detection of the gravitational-wave radiation and also the spectroscopically identified macronova emission (i.e., AT 2017gfo). The prompt emission of this burst, however, is underluminous in comparison with the other short GRBs with known redshift. In this work, we examine whether GRB 170817A is indeed unique. We first show that GRB 130603B/macronova may be the on-axis “analogs” of GRB 170817A/AT 2017gfo, and the extremely dim but long-lasting afterglow emission of GRB 170817A may suggest a low number density ( <?CDATA ∼ 10-5 cm-3?> ) of its circumburst medium and a structured outflow. We then discuss whether GRB 070923, GRB 080121, GRB 090417A, GRB 111005A, and GRB 170817A form a new group of very nearby underluminous GRBs originated from neutron star mergers. If the short events GRB 070923, GRB 080121, and GRB 090417A are indeed at a redshift of <?CDATA ∼ 0.076, 0.046, 0.088?> , respectively, their isotropic energies of the prompt emission are <?CDATA ∼ 1047?> erg and thus comparable to the other two events. The non-detection of optical counterparts of GRB 070923, GRB 080121, GRB 090417A, and GRB 111005A, however, strongly suggests that the macronovae from neutron star mergers are significantly diverse in luminosities or, alternatively, there is another origin channel (for instance, the white dwarf and black hole mergers). We finally suggest that GW170817/GRB 170817A are likely not alone and similar events will be detected by the upgraded/upcoming gravitational-wave detectors and the electromagnetic monitors.