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Localized FRBs are Consistent with Magnetar Progenitors Formed in Core-Collapse Supernovae

Bochenek, Christopher D. and Ravi, Vikram and Dong, Dillon (2020) Localized FRBs are Consistent with Magnetar Progenitors Formed in Core-Collapse Supernovae. . (Unpublished) https://resolver.caltech.edu/CaltechAUTHORS:20201019-085557074

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Abstract

With the localization of fast radio bursts (FRBs) to galaxies similar to the Milky Way and the detection of a bright radio burst from SGR J1935+2154 with energy comparable to extragalactic radio bursts, a magnetar origin for FRBs is evident. By studying the environments of FRBs, evidence for magnetar formation mechanisms not observed in the Milky Way may become apparent. In this paper, we use a sample of FRB host galaxies and a complete sample of core-collapse supernova (CCSN) hosts to determine whether FRB progenitors are consistent with a population of magnetars born in CCSNe. We also compare the FRB hosts to the hosts of hydrogen-poor superluminous supernovae (SLSNe-I) and long gamma-ray bursts (LGRBs) to determine whether the population of FRB hosts is compatible with a population of transients that may be connected to millisecond magnetars. After using a novel approach to scale the stellar masses and star-formation rates of each host galaxy to be statistically representative of z=0 galaxies, we find that the CCSN hosts and FRBs are consistent with arising from the same distribution. Furthermore, the FRB host distribution is inconsistent with the distribution of SLSNe-I and LGRB hosts. With the current sample of FRB host galaxies, our analysis shows that FRBs are consistent with a population of magnetars born through the collapse of giant, highly magnetic stars.


Item Type:Report or Paper (Discussion Paper)
Related URLs:
URLURL TypeDescription
https://arxiv.org/abs/2009.13030arXivDiscussion Paper
ORCID:
AuthorORCID
Bochenek, Christopher D.0000-0003-3875-9568
Ravi, Vikram0000-0002-7252-5485
Dong, Dillon0000-0001-9584-2531
Additional Information:This research was supported by the National Science Foundation under grant AST-1836018. Software: Astropy (Astropy Collaboration et al. 2018).
Group:Astronomy Department
Funders:
Funding AgencyGrant Number
NSFAST-1836018
Subject Keywords:fast radio bursts, neutron stars; supernovae
Record Number:CaltechAUTHORS:20201019-085557074
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20201019-085557074
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:106136
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:20 Oct 2020 18:01
Last Modified:20 Oct 2020 18:01

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