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Constraints on the circumburst environments of short gamma-ray bursts

O'Connor, Brendan and Beniamini, Paz and Kouveliotou, Chryssa (2020) Constraints on the circumburst environments of short gamma-ray bursts. Monthly Notices of the Royal Astronomical Society, 495 (4). pp. 4782-4799. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20200723-122440792

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Abstract

Observational follow up of well localized short gamma-ray bursts (SGRBs) has left 20−30 per cent of the population without a coincident host galaxy association to deep optical and NIR limits (≳26 mag). These SGRBs have been classified as observationally hostless due to their lack of strong host associations. It has been argued that these hostless SGRBs could be an indication of the large distances traversed by the binary neutron star system (due to natal kicks) between its formation and its merger (leading to an SGRB). The distances of GRBs from their host galaxies can be indirectly probed by the surrounding circumburst densities. We show that a lower limit on those densities can be obtained from early afterglow light curves. We find that ≲16 per cent of short GRBs in our sample took place at densities ≲10−4 cm−3. These densities represent the expected range of values at distances greater than the host galaxy’s virial radii. We find that out of the five SGRBs in our sample that have been found to be observationally hostless, none are consistent with having occurred beyond the virial radius of their birth galaxies. This implies one of two scenarios. Either these observationally hostless SGRBs occurred outside of the half-light radius of their host galaxy, but well within the galactic halo, or in host galaxies at moderate to high redshifts (z ≳ 2) that were missed by follow-up observations.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/staa1433DOIArticle
https://arxiv.org/abs/2004.00031arXivDiscussion Paper
ORCID:
AuthorORCID
O'Connor, Brendan0000-0002-9700-0036
Beniamini, Paz0000-0001-7833-1043
Kouveliotou, Chryssa0000-0003-1443-593X
Additional Information:© 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model). Accepted 2020 May 20. Received 2020 May 19; in original form 2020 March 30. The authors thank the referee for their quick response and helpful comments that improved the manuscript. The authors would also like to acknowledge Kenta Hotokezaka, Ehud Nakar, Alexander van der Horst, and Sylvain Guiriec for helpful discussions, and Eleonora Troja for useful comments that improved the manuscript. The authors likewise acknowledge Phillip F. Hopkins for discussions involving the gas density profile of galaxies. The work of BO was supported in part by the National Aeronautics and Space Administration through grants NNX16AB66G, NNX17AB18G, and 80NSSC20K0389. The research of PB was funded by the Gordon and Betty Moore Foundation through Grant GBMF5076. This work made use of data supplied by the UK Swift Science Data Centre at the University of Leicester. The computations were performed on the George Washington University (GWU) Colonial One and Pegasus computer clusters.
Funders:
Funding AgencyGrant Number
NASANNX16AB66G
NASANNX17AB18G
NASA80NSSC20K0389
Gordon and Betty Moore FoundationGBMF5076
Subject Keywords:stars: jet, gamma-ray bursts, neutron star mergers
Issue or Number:4
Record Number:CaltechAUTHORS:20200723-122440792
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200723-122440792
Official Citation:Brendan O’Connor, Paz Beniamini, Chryssa Kouveliotou, Constraints on the circumburst environments of short gamma-ray bursts, Monthly Notices of the Royal Astronomical Society, Volume 495, Issue 4, July 2020, Pages 4782–4799, https://doi.org/10.1093/mnras/staa1433
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:104539
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:23 Jul 2020 19:55
Last Modified:23 Jul 2020 19:55

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