{"title":"BL凸轮*周围的新脉冲变星和食双星","authors":"Ai-Ying Zhou","doi":"10.3847/2515-5172/ad7b2b","DOIUrl":null,"url":null,"abstract":"Based on publicly available Transiting Exoplanet Survey Satellite data, I conducted a regional survey around the SX Phe star BL Cam, spanning a radius of two degrees. This research identified 285 new variables including: 96 δ Scuti stars, 56 γ Doradus stars, 17 eclipsing binary systems with three exhibiting pulsating or rotating components, 3 rotating ellipsoidal variable stars, among others. No new SX Phe stars were identified.","PeriodicalId":74684,"journal":{"name":"Research notes of the AAS","volume":"3 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"New Pulsating Variable Stars and Eclipsing Binaries Around BL Cam*\",\"authors\":\"Ai-Ying Zhou\",\"doi\":\"10.3847/2515-5172/ad7b2b\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Based on publicly available Transiting Exoplanet Survey Satellite data, I conducted a regional survey around the SX Phe star BL Cam, spanning a radius of two degrees. This research identified 285 new variables including: 96 δ Scuti stars, 56 γ Doradus stars, 17 eclipsing binary systems with three exhibiting pulsating or rotating components, 3 rotating ellipsoidal variable stars, among others. No new SX Phe stars were identified.\",\"PeriodicalId\":74684,\"journal\":{\"name\":\"Research notes of the AAS\",\"volume\":\"3 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-09-16\",\"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/ad7b2b\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Research notes of the AAS","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.3847/2515-5172/ad7b2b","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
New Pulsating Variable Stars and Eclipsing Binaries Around BL Cam*
Based on publicly available Transiting Exoplanet Survey Satellite data, I conducted a regional survey around the SX Phe star BL Cam, spanning a radius of two degrees. This research identified 285 new variables including: 96 δ Scuti stars, 56 γ Doradus stars, 17 eclipsing binary systems with three exhibiting pulsating or rotating components, 3 rotating ellipsoidal variable stars, among others. No new SX Phe stars were identified.