A. S. Vinokurov, K. E. Atapin, A. E. Kostenkov, Yu. N. Solovyeva
{"title":"超光速 X 射线源 VII Zw 403 ULX 的 X 射线和光学范围研究","authors":"A. S. Vinokurov, K. E. Atapin, A. E. Kostenkov, Yu. N. Solovyeva","doi":"10.1134/S1063773723120083","DOIUrl":null,"url":null,"abstract":"<p>We present the results of our analysis of the series of X-ray observations, photometric and spectroscopic monitoring for the ultraluminous X-ray source VII Zw 403 ULX (UGC 6456 ULX). Based on a number of indirect signs, we hypothesize that the accretor in this binary system is a neutron star. By analyzing the observed spectrum of this ULX taken during its active state within the framework of the model of a wind coming from the supercritical accretion disk, we have estimated the mass outflow rate to be <span>\\({\\approx}4.0\\times 10^{-5}M_{\\odot}\\)</span> yr<span>\\({}^{-1}\\)</span>.</p>","PeriodicalId":55443,"journal":{"name":"Astronomy Letters-A Journal of Astronomy and Space Astrophysics","volume":"49 12","pages":"787 - 795"},"PeriodicalIF":1.1000,"publicationDate":"2024-03-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Investigation of the Ultraluminous X-ray Source VII Zw 403 ULX in the X-ray and Optical Ranges\",\"authors\":\"A. S. Vinokurov, K. E. Atapin, A. E. Kostenkov, Yu. N. Solovyeva\",\"doi\":\"10.1134/S1063773723120083\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>We present the results of our analysis of the series of X-ray observations, photometric and spectroscopic monitoring for the ultraluminous X-ray source VII Zw 403 ULX (UGC 6456 ULX). Based on a number of indirect signs, we hypothesize that the accretor in this binary system is a neutron star. By analyzing the observed spectrum of this ULX taken during its active state within the framework of the model of a wind coming from the supercritical accretion disk, we have estimated the mass outflow rate to be <span>\\\\({\\\\approx}4.0\\\\times 10^{-5}M_{\\\\odot}\\\\)</span> yr<span>\\\\({}^{-1}\\\\)</span>.</p>\",\"PeriodicalId\":55443,\"journal\":{\"name\":\"Astronomy Letters-A Journal of Astronomy and Space Astrophysics\",\"volume\":\"49 12\",\"pages\":\"787 - 795\"},\"PeriodicalIF\":1.1000,\"publicationDate\":\"2024-03-22\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Astronomy Letters-A Journal of Astronomy and Space Astrophysics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.1134/S1063773723120083\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomy Letters-A Journal of Astronomy and Space Astrophysics","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1134/S1063773723120083","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
摘要
摘要我们介绍了对超亮 X 射线源 VII Zw 403 ULX（UGC 6456 ULX）的一系列 X 射线观测、光度测量和光谱监测的分析结果。根据一些间接迹象，我们推测这个双星系统中的吸积器是一颗中子星。通过在来自超临界吸积盘的风的模型框架内分析这颗ULX在其活跃状态下的观测光谱，我们估计其质量流出率为（{}^{-1}/4.0/times 10^{-5}M_{\odot}\) yr\({}^{-1}\).
Investigation of the Ultraluminous X-ray Source VII Zw 403 ULX in the X-ray and Optical Ranges
We present the results of our analysis of the series of X-ray observations, photometric and spectroscopic monitoring for the ultraluminous X-ray source VII Zw 403 ULX (UGC 6456 ULX). Based on a number of indirect signs, we hypothesize that the accretor in this binary system is a neutron star. By analyzing the observed spectrum of this ULX taken during its active state within the framework of the model of a wind coming from the supercritical accretion disk, we have estimated the mass outflow rate to be \({\approx}4.0\times 10^{-5}M_{\odot}\) yr\({}^{-1}\).
期刊介绍：
Astronomy Letters is an international peer reviewed journal that publishes the results of original research on all aspects of modern astronomy and astrophysics including high energy astrophysics, cosmology, space astronomy, theoretical astrophysics, radio astronomy, extragalactic astronomy, stellar astronomy, and investigation of the Solar system.
京公网安备 11010802042870号
京ICP备2023020795号-1
分享
求助内容：
应助结果提醒方式：
扫码关注我们
