A High-Resolution View of Fast Radio Burst Host Environments
Alexandra Mannings,Wen-fai Fong,Sunil Simha,J. Xavier Prochaska,Marc Rafelski,Charles D. Kilpatrick,Nicolas Tejos,Kasper E. Heintz,Shivani Bhandari,Cherie K. Day,Adam Deller,Stuart D. Ryder,Ryan Shannon,Shriharsh P. Tendulkar +13 more
TLDR
In this article, the authors quantify the spatial distribution and locations of fast radio burst (FRB) host galaxies with sub-arcsecond localizations, including the hosts of three known repeating FRBs.Abstract:
We present Hubble Space Telescope (HST/WFC3) ultraviolet and infrared observations of eight fast radio burst (FRB) host galaxies with sub-arcsecond localizations, including the hosts of three known repeating FRBs. We quantify their spatial distributions and locations with respect to their host galaxy light distributions, finding that they occur at moderate host normalized-offsets of 1.4 $r_e$ ([0.6,2.1] $r_e$; 68% interval), occur on fainter regions of their hosts in terms of IR light, but overall trace the radial distribution of IR light in their galaxies. The FRBs in our tested distribution do not clearly trace the distributions of any other transient population with known progenitors, and are statistically distinct from the locations of LGRBs, H-poor SLSNe, SGRBs, and Ca-rich transients. We further find that most FRBs are not in regions of elevated local star formation rate and stellar mass surface densities in comparison to the mean global values of their hosts. We also place upper limits to the IR flux at the FRB positions of $m_{\rm IR}\gtrsim\!24.8-27.6$~AB~mag, constraining both satellite and background galaxies to luminosities well below the host luminosity of FRB121102. We find that 5/8 FRB hosts exhibit clear spiral arm features in IR light, and that the positions of all well-localized FRBs located in such hosts are consistent with their spiral arms, although not on their brightest regions. Our results do not strongly support the primary progenitor channel of FRBs being connected either with the most massive (stripped-envelope) stars, or with events which require kicks and long delay times (neutron star mergers).read more
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Journal ArticleDOI
Periodic Fast Radio Bursts from Luminous X-ray Binaries
Navin Sridhar,Brian D. Metzger,Paz Beniamini,Ben Margalit,Mathieu Renzo,Lorenzo Sironi,Konstantinos Kovlakas +6 more
TL;DR: In this article, the authors proposed a new scenario in which fast radio bursts are powered by short-lived relativistic outflows from accreting black holes or neutron stars, which propagate into the cavity of the pre-existing (quiescent'') jet.
Journal ArticleDOI
Chronicling the Host Galaxy Properties of the Remarkable Repeating FRB 20201124A
W. Fong,Y. Dong,Y. Dong,Joel Leja,Shivani Bhandari,Cherie K. Day,Cherie K. Day,Adam T. Deller,Pravir Kumar,J. Xavier Prochaska,J. Xavier Prochaska,D. R. Scott,Keith W. Bannister,Tarraneh Eftekhari,Alexa C. Gordon,Kasper E. Heintz,Kasper E. Heintz,C. W. James,Charles D. Kilpatrick,Elizabeth K. Mahony,Alicia Rouco Escorial,Stuart D. Ryder,Ryan Shannon,Nicolas Tejos +23 more
TL;DR: In this paper, the authors presented the Australian Square Kilometre Array Pathfinder (ASKAP) localization and follow-up observations of the host galaxy of the repeating FRB 20201124A, the fifth such extragalactic repeating fast radio burst (FRB) with an identified host.
Posted Content
The host galaxy and persistent radio counterpart of FRB 20201124A
Vikram Ravi,Casey J. Law,D. Z. Li,Kshitij Aggarwal,Sarah Burke-Spolaor,Liam Connor,T. Joseph W. Lazio,Dana Simard,Jean J. Somalwar,Shriharsh P. Tendulkar +9 more
TL;DR: In this paper, the authors presented a localisation of the repeating source FRB 20201124A, and its association with a host galaxy (SDSS J050803.48+260338.0, z=0.098) and persistent radio source.
Journal ArticleDOI
A Local Universe Host for the Repeating Fast Radio Burst FRB 20181030A
Mohit Bhardwaj,A. Yu. Kirichenko,D. Michilli,Y. D. Mayya,V. M. Kaspi,Bryan Gaensler,M. Rahman,Shriharsh P. Tendulkar,Emmanuel Fonseca,A. Josephy,Calvin Leung,M. Merryfield,Emily Petroff,Ziggy Pleunis,Pranav Sanghavi,Paul Scholz,Kyung-Hoon Shin,Kendrick M. Smith,Ingrid H. Stairs +18 more
TL;DR: In this article, the authors reported on the host association of FRB 20181030A, a repeating fast radio burst (FRB) with a low dispersion measure (DM, 103.5 pc cm$-3}$) discovered by CHIME/FRB Collaboration et al. Using baseband voltage data saved for its repeat bursts, they localize the FRB to a sky area of 5.3 sq. arcmin (90% confidence).
Journal ArticleDOI
A nearby repeating fast radio burst in the direction of M81
Mohit Bhardwaj,Bryan Gaensler,V. M. Kaspi,T. L. Landecker,R. Mckinven,Daniele Michilli,Ziggy Pleunis,Shriharsh P. Tendulkar,B. C. Andersen,P. J. Boyle,Tomas Cassanelli,P. Chawla,A. Cook,M. A. Dobbs,Emmanuel Fonseca,Jane F. Kaczmarek,Calvin Leung,Kiyoshi Masui,Moritz Münchmeyer,Cherry Ng,M. Rafiei-Ravandi,P. Scholz,Kyung-Hoon Shin,K. M. Smith,I. H. Stairs,A. V. Zwaniga +25 more
TL;DR: In this article, a repeating fast radio burst (FRB) with low dispersion measure (DM) was detected by the Canadian Hydrogen Intensity Mapping Experiment (CHIME)/FRB project.
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TL;DR: In this article, the authors present a cosmological analysis based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation.
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