CHIME又看到在M81那儿一个重复的FRB

CHIME又看到在M81那儿一个重复的FRB

arXiv:2103.01295 [pdf, other]

A nearby repeating fast radio burst in the direction of M81

M. Bhardwaj, B. M. Gaensler, V. M. Kaspi, T. L. Landecker, R. Mckinven, D. Michilli, Z. Pleunis, S. P. Tendulkar, B. C. Andersen, P. J. Boyle, T. Cassanelli, P. Chawla, A. Cook, M. Dobbs, E. Fonseca, J. Kaczmarek, C. Leung, K. Masui, M. Münchmeyer, C. Ng, M. Rafiei-Ravandi, P. Scholz, K. Shin, K. M. Smith, I. H. Stairs, A. V. Zwaniga

Comments: In press, ApJL; comments still welcome

Subjects: High Energy Astrophysical Phenomena (astro-ph.HE); Astrophysics of Galaxies (astro-ph.GA)

We report on the discovery of FRB 20200120E, a repeating fast radio burst (FRB) with low dispersion measure (DM), detected by the Canadian Hydrogen Intensity Mapping Experiment (CHIME)/FRB project. The source DM of 87.82 pc cm−3 is the lowest recorded from an FRB to date, yet is significantly higher than the maximum expected from the Milky Way interstellar medium in this direction (~ 50 pc cm−3). We have detected three bursts and one candidate burst from the source over the period 2020 January-November. The baseband voltage data for the event on 2020 January 20 enabled a sky localization of the source to within ≃ 14 sq. arcmin (90% confidence). The FRB localization is close to M81, a spiral galaxy at a distance of 3.6 Mpc. The FRB appears on the outskirts of M81 (projected offset ∼ 20 kpc) but well inside its extended HI and thick disks. We empirically estimate the probability of chance coincidence with M81 to be <10−2. However, we cannot reject a Milky Way halo origin for the FRB. Within the FRB localization region, we find several interesting cataloged M81 sources and a radio point source detected in the Very Large Array Sky Survey (VLASS). We searched for prompt X-ray counterparts in Swift/BAT and Fermi/GBM data, and for two of the FRB 20200120E bursts, we rule out coincident SGR 1806−20-like X-ray bursts. Due to the proximity of FRB 20200120E, future follow-up for prompt multi-wavelength counterparts and sub-arcsecond localization could be constraining of proposed FRB models.

来源： https://arxiv.org/list/astro-ph/new

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