{"@context":{"@vocab":"https://cir.nii.ac.jp/schema/1.0/","rdfs":"http://www.w3.org/2000/01/rdf-schema#","dc":"http://purl.org/dc/elements/1.1/","dcterms":"http://purl.org/dc/terms/","foaf":"http://xmlns.com/foaf/0.1/","prism":"http://prismstandard.org/namespaces/basic/2.0/","cinii":"http://ci.nii.ac.jp/ns/1.0/","datacite":"https://schema.datacite.org/meta/kernel-4/","ndl":"http://ndl.go.jp/dcndl/terms/","jpcoar":"https://github.com/JPCOAR/schema/blob/master/2.0/"},"@id":"https://cir.nii.ac.jp/crid/1363101969240923904.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.3847/1538-4357/ab3e3f"}},{"identifier":{"@type":"URI","@value":"https://iopscience.iop.org/article/10.3847/1538-4357/ab3e3f/pdf"}},{"identifier":{"@type":"URI","@value":"https://iopscience.iop.org/article/10.3847/1538-4357/ab3e3f"}},{"identifier":{"@type":"DOI","@value":"10.48550/arxiv.1908.09269"}},{"identifier":{"@type":"HANDLE","@value":"10900/103344"}},{"identifier":{"@type":"HANDLE","@value":"1959.7/uws:55062"}},{"identifier":{"@type":"HANDLE","@value":"2440/122815"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"A Supernova Remnant Counterpart for HESS J1832−085"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title>\n               <jats:p>We examine the new Galactic supernova remnant (SNR) candidate, G23.11+0.18, as seen by the Murchison Widefield Array radio telescope. We describe the morphology of the candidate and find a spectral index of −0.63 ± 0.05 in the 70–170 MHz domain. Coincident TeV gamma-ray detection in High Energy Stereoscopic System (HESS) data supports the SNR nature of G23.11+0.18 and suggests that G23.11+0.18 is accelerating particles beyond TeV energies, thus making this object a promising new cosmic-ray hadron source candidate. The remnant cannot be seen in current optical, infrared and X-ray data sets. We do find, however, a dip in CO-traced molecular gas at a line-of-sight velocity of ∼85 km s<jats:sup>−1</jats:sup>, suggesting the existence of a G23.11+0.18 progenitor wind-blown bubble. Furthermore, the discovery of molecular gas clumps at a neighboring velocity toward HESS J1832−085 adheres to the notion that a hadronic gamma-ray production mechanism is plausible toward the north of the remnant. Based on these morphological arguments, we propose an interstellar medium association for G23.11+0.18 at a kinematic distance of 4.6 ± 0.8 kpc.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1383101969240923910","@type":"Researcher","foaf:name":[{"@value":"Nigel I. Maxted"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240924165","@type":"Researcher","foaf:name":[{"@value":"M. D. Filipović"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240924038","@type":"Researcher","foaf:name":[{"@value":"N. Hurley-Walker"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240923917","@type":"Researcher","foaf:name":[{"@value":"I. Bojičić"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240923908","@type":"Researcher","foaf:name":[{"@value":"G. P. Rowell"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240924036","@type":"Researcher","foaf:name":[{"@value":"F. Haberl"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240924033","@type":"Researcher","foaf:name":[{"@value":"A. J. Ruiter"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240924040","@type":"Researcher","foaf:name":[{"@value":"I. R. Seitenzahl"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240924032","@type":"Researcher","foaf:name":[{"@value":"F. Panther"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240924039","@type":"Researcher","foaf:name":[{"@value":"G. F. Wong"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240923914","@type":"Researcher","foaf:name":[{"@value":"C. Braiding"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240923779","@type":"Researcher","foaf:name":[{"@value":"M. Burton"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240924167","@type":"Researcher","foaf:name":[{"@value":"G. Pühlhofer"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240924034","@type":"Researcher","foaf:name":[{"@value":"H. Sano"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240923777","@type":"Researcher","foaf:name":[{"@value":"Y. Fukui"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240923911","@type":"Researcher","foaf:name":[{"@value":"M. Sasaki"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240923781","@type":"Researcher","foaf:name":[{"@value":"W. Tian"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240924044","@type":"Researcher","foaf:name":[{"@value":"H. Su"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240924037","@type":"Researcher","foaf:name":[{"@value":"X. Cui"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240923906","@type":"Researcher","foaf:name":[{"@value":"D. Leahy"}]},{"@id":"https://cir.nii.ac.jp/crid/1383101969240924163","@type":"Researcher","foaf:name":[{"@value":"P. J. Hancock"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"0004637X"},{"@type":"EISSN","@value":"15384357"}],"prism:publicationName":[{"@value":"The Astrophysical Journal"}],"dc:publisher":[{"@value":"American Astronomical Society"}],"prism:publicationDate":"2019-11-07","prism:volume":"885","prism:number":"2","prism:startingPage":"129"},"reviewed":"false","dc:rights":["https://iopscience.iop.org/page/copyright","https://iopscience.iop.org/info/page/text-and-data-mining"],"url":[{"@id":"https://iopscience.iop.org/article/10.3847/1538-4357/ab3e3f/pdf"},{"@id":"https://iopscience.iop.org/article/10.3847/1538-4357/ab3e3f"}],"createdAt":"2019-11-07","modifiedAt":"2024-01-12","foaf:topic":[{"@id":"https://cir.nii.ac.jp/all?q=supernova%20remnants","dc:title":"supernova remnants"},{"@id":"https://cir.nii.ac.jp/all?q=High%20Energy%20Astrophysical%20Phenomena%20(astro-ph.HE)","dc:title":"High Energy Astrophysical Phenomena (astro-ph.HE)"},{"@id":"https://cir.nii.ac.jp/all?q=gamma%20ray%20sources","dc:title":"gamma ray sources"},{"@id":"https://cir.nii.ac.jp/all?q=FOS:%20Physical%20sciences","dc:title":"FOS: Physical sciences"},{"@id":"https://cir.nii.ac.jp/all?q=530","dc:title":"530"},{"@id":"https://cir.nii.ac.jp/all?q=520","dc:title":"520"},{"@id":"https://cir.nii.ac.jp/all?q=interstellar%20molecules","dc:title":"interstellar molecules"},{"@id":"https://cir.nii.ac.jp/all?q=XXXXXX%20-%20Unknown","dc:title":"XXXXXX - Unknown"},{"@id":"https://cir.nii.ac.jp/all?q=galactic%20cosmic%20rays","dc:title":"galactic cosmic rays"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20High%20Energy%20Astrophysical%20Phenomena","dc:title":"Astrophysics - High Energy Astrophysical Phenomena"},{"@id":"https://cir.nii.ac.jp/all?q=interstellar%20matter","dc:title":"interstellar matter"}],"project":[{"@id":"https://cir.nii.ac.jp/crid/1040000782015382528","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"19H05075"},{"@type":"JGN","@value":"JP19H05075"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PUBLICLY-19H05075/"}],"notation":[{"@language":"ja","@value":"超新星残骸に付随するフィラメント状分子雲の探究"},{"@language":"en","@value":"Pursuit of molecular filaments associated with supernova remnants"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000782439701376","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"15H05694"},{"@type":"JGN","@value":"JP15H05694"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-15H05694/"}],"notation":[{"@language":"ja","@value":"星間水素の精密定量による新たな星間物質像の構築"},{"@language":"en","@value":"Innovation of the “Interstellar medium” by accurate measurements of the interstellar hydrogen"}]},{"@id":"https://cir.nii.ac.jp/crid/1040282256998833024","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"19K14758"},{"@type":"JGN","@value":"JP19K14758"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-19K14758/"}],"notation":[{"@language":"ja","@value":"近傍系外銀河の超新星残骸に付随する星間雲"},{"@language":"en","@value":"Interstellar gas associated with supernova remnants in the nearby galaxies"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050845763745230592","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Possible Evidence for Cosmic-Ray Acceleration in the Type Ia SNR RCW 86: Spatial Correlation between TeV Gamma-Rays and Interstellar Atomic Protons"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002216521274752","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Dense Gas Towards the RX J1713.7–3946 Supernova Remnant"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002217425229440","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"INTERSTELLAR PROTONS IN THE TeV γ-RAY SNR HESS J1731-347: POSSIBLE EVIDENCE FOR THE COEXISTENCE OF HADRONIC AND LEPTONIC γ-RAYS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002217600365952","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Probing the local environment of the supernova remnant HESS J1731−347 with CO and CS observations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144438806400","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Detection of the Characteristic Pion-Decay Signature in Supernova Remnants"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144558356480","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Observations of the Crab nebula with HESS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283690992098816","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Interstellar gas and X-rays toward the Young supernova remnant RCW 86; 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