A non-repeating fast radio burst in a dwarf host galaxy

Autor: Bhandari, Shivani, Gordon, Alexa C., Scott, Danica R., Marnoch, Lachlan, Sridhar, Navin, Kumar, Pravir, James, Clancy W., Qiu, Hao, Bannister, Keith W., Deller, Adam T., Eftekhari, Tarraneh, Fong, Wen-fai, Glowacki, Marcin, Prochaska, J. Xavier, Ryder, Stuart D., Shannon, Ryan M., Simha, Sunil
Rok vydání: 2022
Předmět:
Zdroj: ApJ 948 67 (2023)
Druh dokumentu: Working Paper
DOI: 10.3847/1538-4357/acc178
Popis: We present the discovery of as-of-yet non-repeating Fast Radio Burst (FRB), FRB 20210117A, with the Australian Square Kilometer Array Pathfinder (ASKAP) as a part of the Commensal Real-time ASKAP Fast Transients (CRAFT) Survey. The sub-arcsecond localization of the burst led to the identification of its host galaxy at a $z=0.214(1)$. This redshift is much lower than what would be expected for a source dispersion measure (DM) of 729 pc cm$^{-3}$, given typical contributions from the intergalactic medium and the host galaxy. Optical observations reveal the host to be a dwarf galaxy with little on-going star formation, very different to the dwarf host galaxies of known repeating FRBs 20121102A, and 20190520B. We find an excess DM contribution from the host and attribute it to the FRB's local environment. We do not find any radio emission from the FRB site or host galaxy. The low magnetized environment and lack of a persistent radio source (PRS) indicate that the FRB source is older than those found in other dwarf host galaxies, and establish the diversity of FRB sources in dwarf galaxy environments. We find our observations to be fully consistent with the hypernebula model, where the FRB is powered by accretion-jet from a hyper-accreting black hole. Finally, our high-time resolution analysis reveals burst characteristics similar to those seen in repeating FRBs. We encourage follow-up observations of FRB 20210117A to establish any repeating nature.
Comment: 15 pages, 9 figures, 2 Tables
Databáze: arXiv
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