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Massive stars dying alone: the remote environment of supernova 2010jp and its associated late-time source

Corgan, Austin and Smith, Nathan and Andrews, Jennifer E. and Filippenko, Alexei V. and Van Dyk, Schuyler D. (2022) Massive stars dying alone: the remote environment of supernova 2010jp and its associated late-time source. Monthly Notices of the Royal Astronomical Society, 510 (1). pp. 1-10. ISSN 0035-8711. doi:10.1093/mnras/stab2892. https://resolver.caltech.edu/CaltechAUTHORS:20220309-964969000

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Abstract

We present late-time images of the site of the peculiar jet-driven Type IIn supernova (SN) 2010jp, including Hubble Space Telescope images taken 2–5 yr post-explosion and deep ground-based images over a similar time. These are used to characterize its unusually remote environment and to constrain the progenitor’s initial mass and age. The position of SN 2010jp is found to reside along a chain of diffuse starlight that is probably an outer spiral arm or tidal tail of the interacting galaxy pair NGC 2207/IC 2163. There is one bright H ii region projected within 1 kpc, and there is faint extended H α emission immediately surrounding the continuum source at the position of SN 2010jp, which has M_(F555W) = −7.7 ± 0.2 mag. In principle, the lingering light could arise from late-time circumstellar material (CSM) interaction, an evolved supergiant, a host star cluster, or some combination of these. Steady flux over 3 yr and a lack of strong, spatially unresolved H α emission make ongoing CSM interaction unlikely. If an evolved supergiant dominates, its observed luminosity implies an initial mass ≾ 22 M_⊙ and an age ≳ 8 Myr. If the source is a star cluster, then its colour and absolute magnitude imply an age of 8–13 Myr and a modest cluster initial mass of log(M/M_⊙) = 3.6–3.8. Extended H α emission out to a radius of ∼30 pc reveals a faint evolved H ii region, pointing to recent star formation with at least one late O-type star. Based on these various clues, we conclude that the progenitor of SN 2010jp had a likely initial mass of 18–22 M_⊙.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/stab2892DOIArticle
https://arxiv.org/abs/2201.02657arXivDiscussion Paper
ORCID:
AuthorORCID
Smith, Nathan0000-0001-5510-2424
Andrews, Jennifer E.0000-0003-0123-0062
Filippenko, Alexei V.0000-0003-3460-0103
Van Dyk, Schuyler D.0000-0001-9038-9950
Additional Information:© 2021 The Author(s) Published by Oxford University Press on behalf of 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 2021 September 30. Received 2021 September 3; in original form 2021 March 3. We thank an anonymous referee for helpful suggestions. Based on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute (STScI), which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. Support was provided by NASA through grants GO-13029 and GO-13787 from STScI. AVF is also grateful for financial support from the TABASGO Foundation, the Miller Institute for Basic Research in Science (U.C. Berkeley, where he is a Senior Miller Fellow), the Christopher R. Redlich Fund, and many individual donors. Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes. This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile. Figures were created with ANACONDA (Anaconda Software Distribution, computer software, ver. 2-2.4.0, 2016 November; https://anaconda.com) using the following PYTHON packages: ASTROPY [Astropy Collaboration 2013; (doi: 10.3847/1538-3881/aabc4f)], MATPLOTLIB (doi: 10.1109/MCSE.2007.55), and NUMPY (doi: 10.1109/MCSE.2011.37). Facilities: HST (WFC3), Magellan (IMACS). DATA AVAILABILITY. The data underlying this article will be shared on reasonable request to the corresponding author. HST data are non-proprietary and available from the public archive.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASANAS 5-26555
NASAGO-13787
NASAGO-13029
TABASGO FoundationUNSPECIFIED
Miller Institute for Basic Research in ScienceUNSPECIFIED
Christopher R. Redlich FundUNSPECIFIED
Subject Keywords:blue stragglers, circumstellar matter, stars: evolution, supernovae: general, supernovae: individual (SN 2010jp)
Issue or Number:1
DOI:10.1093/mnras/stab2892
Record Number:CaltechAUTHORS:20220309-964969000
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20220309-964969000
Official Citation:Austin Corgan, Nathan Smith, Jennifer Andrews, Alexei V Filippenko, Schuyler D Van Dyk, Massive stars dying alone: the remote environment of supernova 2010jp and its associated late-time source, Monthly Notices of the Royal Astronomical Society, Volume 510, Issue 1, February 2022, Pages 1–10, https://doi.org/10.1093/mnras/stab2892
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:113838
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:11 Mar 2022 15:55
Last Modified:11 Mar 2022 15:55

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