Zachary J. Smeaton, M. D. Filipović, B. Koribalski, S. Lazarević, R. Alsaberi, Werner Becker, K. Dage, Yjan A. Gordon, Andrew M. Hopkins, R. Kothes, D. Leahy, Ana Mitras̆inović
{"title":"ASKAP-EMU Discovery of New Galactic SNR Candidate: Unicycle (G312.65+2.87)","authors":"Zachary J. Smeaton, M. D. Filipović, B. Koribalski, S. Lazarević, R. Alsaberi, Werner Becker, K. Dage, Yjan A. Gordon, Andrew M. Hopkins, R. Kothes, D. Leahy, Ana Mitras̆inović","doi":"10.3847/2515-5172/ad5309","DOIUrl":null,"url":null,"abstract":"We present the serendipitous discovery of a low surface brightness Galactic supernova remnant candidate, Unicycle (G312.65+2.87). Unicycle was initially discovered in the Evolutionary Map of the Universe large-scale radio survey at 943.5 MHz. We measure a diffuse shell (D = 288″ × 300″) and an integrated flux density of S I 944 MHz = 150 ± 20 mJy. We estimate the most likely intrinsic diameters of 30 < D < 36 pc or 42 < D < 47 pc, corresponding to distances of 10 < d < 12 kpc or 14 < d < 16 kpc, placing it within either the Scutum–Centaurus or outer Sagittarius spiral arms.","PeriodicalId":74684,"journal":{"name":"Research notes of the AAS","volume":"91 8","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-06-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Research notes of the AAS","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.3847/2515-5172/ad5309","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
We present the serendipitous discovery of a low surface brightness Galactic supernova remnant candidate, Unicycle (G312.65+2.87). Unicycle was initially discovered in the Evolutionary Map of the Universe large-scale radio survey at 943.5 MHz. We measure a diffuse shell (D = 288″ × 300″) and an integrated flux density of S I 944 MHz = 150 ± 20 mJy. We estimate the most likely intrinsic diameters of 30 < D < 36 pc or 42 < D < 47 pc, corresponding to distances of 10 < d < 12 kpc or 14 < d < 16 kpc, placing it within either the Scutum–Centaurus or outer Sagittarius spiral arms.