D. Marchev, K. Stoyanov, V. Marchev, R. Zamanov, B. Borisov, Doroteq Vasileva, T. Atanasova, Nataliya Pavlova
{"title":"用于共生恒星MWC 560的光学闪烁","authors":"D. Marchev, K. Stoyanov, V. Marchev, R. Zamanov, B. Borisov, Doroteq Vasileva, T. Atanasova, Nataliya Pavlova","doi":"10.2478/asn-2022-0017","DOIUrl":null,"url":null,"abstract":"Abstract This study is based on observations of MWC560 during the last two observational seasons (2020/2021 and 2021/2022). Other than looking for flickering we were interested in following the variability of brightness in the same period. Looking for similarities in the spectra with other types of stars is also of great interest to us because it could help clarify the stellar configuration of such objects. Our observations during the last two observational seasons of MWC560 confirm the absence of flickering. From the similarities of the gathered spectra of XX Oph and MWC560 we assume that the components in XX Oph are a red giant and a white dwarf, which are also surrounded by a common shell.","PeriodicalId":7171,"journal":{"name":"Acta Scientifica Naturalis","volume":"9 1","pages":"1 - 9"},"PeriodicalIF":0.0000,"publicationDate":"2022-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"For optical flickering in symbiotic star MWC 560\",\"authors\":\"D. Marchev, K. Stoyanov, V. Marchev, R. Zamanov, B. Borisov, Doroteq Vasileva, T. Atanasova, Nataliya Pavlova\",\"doi\":\"10.2478/asn-2022-0017\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Abstract This study is based on observations of MWC560 during the last two observational seasons (2020/2021 and 2021/2022). Other than looking for flickering we were interested in following the variability of brightness in the same period. Looking for similarities in the spectra with other types of stars is also of great interest to us because it could help clarify the stellar configuration of such objects. Our observations during the last two observational seasons of MWC560 confirm the absence of flickering. From the similarities of the gathered spectra of XX Oph and MWC560 we assume that the components in XX Oph are a red giant and a white dwarf, which are also surrounded by a common shell.\",\"PeriodicalId\":7171,\"journal\":{\"name\":\"Acta Scientifica Naturalis\",\"volume\":\"9 1\",\"pages\":\"1 - 9\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2022-11-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Acta Scientifica Naturalis\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.2478/asn-2022-0017\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Acta Scientifica Naturalis","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.2478/asn-2022-0017","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Abstract This study is based on observations of MWC560 during the last two observational seasons (2020/2021 and 2021/2022). Other than looking for flickering we were interested in following the variability of brightness in the same period. Looking for similarities in the spectra with other types of stars is also of great interest to us because it could help clarify the stellar configuration of such objects. Our observations during the last two observational seasons of MWC560 confirm the absence of flickering. From the similarities of the gathered spectra of XX Oph and MWC560 we assume that the components in XX Oph are a red giant and a white dwarf, which are also surrounded by a common shell.
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