A systematic study of evolved supernova remnants in the large and small Magellanic Clouds with Suzaku

Takeuchi Yoko; Yamaguchi Hiroya; Tamagawa Toru

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A systematic study of evolved supernova remnants in the large and small Magellanic Clouds with Suzaku

机译：带有朱雀星系的大小麦哲伦星云中演化的超新星残留物的系统研究

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Identifyingtheorigintype(i.e.,Typea€‰Iaorcore-collapse)ofsupernovaremnants(SNRs)iscrucialtodeterminingtheratesofsupernova(SN)explosionsinagalaxy,whichisakeytounderstandingitsrecentchemicalevolution.However,evolvedSNRsintheso-calledSedovphasearedominatedbytheswept-upinterstellarmedium(ISM),makingitdifficulttodeterminetheirejectacompositionandthusSNtype.HerewepresentasystematicX-raystudyofnineevolvedSNRsintheMagellanicClouds,DEM??L238,DEM??L249,0534a?’69.9,0548a?’70.4,B0532a?’71.0,B0532a?’67.5,0103a?’72.6,0049a?’73.6,and0104a?’72.3,usingarchivaldataoftheSuzakusatellite.AlthoughSuzakudoesnotspatiallyresolvetheSNejectafromtheswept-upISMduetothelimitedangularresolution,itsexcellentenergyresolutionhasenabledclearseparationofemissionlinesinthesoftX-rayband.Thisleadstothefindingthatthea€?spatiallyintegrateda€?spectraoftheevolved(a??104a€‰yr)SNRsarestillsignificantlycontributedbyemissionfromtheejectaatenergiesaround1a€‰keV.TheFe/Nemassratios,determinedmainlyfromthewell-resolvedFeL-shellandNeK-shelllines,clearlydividetheobservedSNRsintotheTypea€‰Iaandcore-collapsegroups,confirmingsomeprevioustypingmadebyChandraobservationsthathadutilizeditsextremelyhighangularresolution.ThisdemonstratesthatspatiallyintegratedX-rayspectraofoldSNRscanalsobeusedtodiscriminatetheirprogenitortype,whichwouldbehelpfulforfuturesystematicstudiesofextragalacticSNRswithASTRO-Handbeyond.

机译：Identifyingtheorigintype（即，类型a€‰Iaorcore塌陷）ofsupernovaremnants（信噪比）iscrucialtodeterminingtheratesofsupernova（SN）explosionsinagalaxy，whichisakeytounderstandingitsrecentchemicalevolution.However，evolvedSNRsintheso-calledSedovphasearedominatedbytheswept-upinterstellarmedium（ISM），makingitdifficulttodeterminetheirejectacompositionandthusSNtype.HerewepresentasystematicX-raystudyofnineevolvedSNRsintheMagellanicClouds，DEM ?? L238，DEM ?? L249， 0534a？'69 .9,0548a？'70 1.4，B0532a？'71 2.0，B0532a？'67 .5,0103a？'72 .6,0049a？'73 .6 and0104a？'72 3，usingarchivaldataoftheSuzakusatellite.AlthoughSuzakudoesnotspatiallyresolvetheSNejectafromtheswept-upISMduetothelimitedangularresolution，itsexcellentenergyresolutionhasenabledclearseparationofemissionlinesinthesoftX-rayband.Thisleadstothefindingthatthea€？spatiallyintegrateda€演化出的频谱（约104 ayr年）信噪比仍主要由1keV能量附近的喷射能量引起。Fe/ Nemassratios主要由分辨良好的FeL壳和NeK-s决定。地狱，明确地将观察到的SNR划分为I类和核心崩溃组，确认使用了极高角度分辨率的钱德拉观测所进行的一些先前的打字。

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《PASJ: Publications of the Astronomical Society of Japan》 |2016年第sp1期|共页
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Takeuchi Yoko; Yamaguchi Hiroya; Tamagawa Toru;
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1. SUPERNOVA REMNANTS IN THE MAGELLANIC CLOUDS. IV. X-RAY EMISSION FROM THE LARGEST SUPERNOVA REMNANT IN THE LARGE MAGELLANIC CLOUD [J] . R. M. WILLIAMS, Y.-H. CHU, J. R. DICKEL, The Astrophysical journal . 2004,第2Pt1期

机译：麦哲伦云中的超新星遗迹。 IV。大麦哲伦云中最大的超新星遗迹的X射线发射
2. SUPERNOVA REMNANTS IN THE MAGELLANIC CLOUDS. IV. X-RAY EMISSION FROM THE LARGEST SUPERNOVA REMNANT IN THE LARGE MAGELLANIC CLOUD [J] . R. M. WILLIAMS, Y.-H. CHU, J. R. DICKEL, The Astrophysical journal . 2004,第2Pt1期

机译：麦哲伦云中的超新星遗迹。 IV。大麦哲伦云中最大的超新星遗迹的X射线发射
3. Supernova remnants in the magellanic clouds. III. an X-ray atlas of large magellanic cloud supernova remnants [J] . Rosa Murphy Williams, You-Hua Chu, John R. Dickel, The Astrophysical Journal. Supplement Series . 1999,第2期

机译：麦哲伦星云中的超新星残余。三，麦哲伦星云超新星遗迹的X射线地图集
4. Suzaku Observation of the Supernova Remnant N23 in the Large Magellanic Cloud [C] . Kentaro Someya, Aya Bamba, Manabu Ishida, Suzaku international conference on energetic cosmos : from Suzaku to ASTRO-H . 2010

机译：Suzaku观察大型麦哲伦云中超新星残余N23
5. A Chandra Study of Supernova Remnants in the Large and Small Magellanic Clouds. [D] . Schenck, Andrew Corey. 2017

机译：麦哲伦星云中超新星残留物的Chandra研究。
6. Chandra’s First Decade of Discovery Special Feature: X-ray studies of supernova remnants: A different view of supernova explosions [O] . Carles Badenes 2010

机译：钱德拉发现的第一个十年特别报道：超新星残留物的X射线研究：超新星爆炸的不同视角
7. Supernova Remnants in the Magellanic Clouds. III. an X-Ray Atlas of Large Magellanic Cloud Supernova Remnants [O] . R. M. Williams, Y. -h. Chu, J. R. Dickel, 1999

机译：麦哲伦星云中的超新星遗迹。 III。大麦哲伦云超新星遗迹的X射线地图集

A systematic study of evolved supernova remnants in the large and small Magellanic Clouds with Suzaku

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