A long-term UBVRI photometric study of the pre-main sequence star V350 Cep

• 作 者: Sunay Ibryamov Evgeni Semkov S
• 机 构: InstituteofAstronomyandNationalAstronomicalObservatory
• 出 处: 天文和天体物理学研究：英文版
• 发表日期: 2014年10期
• 关键词: 光度变化 主序星 测光观测 观测周期 委员会 MAG 数据表 低振幅 stars pre-main sequence -- stars variable T
• 基金项目: This study was partly supported by ESF and the Bulgarian Ministry of Education and Science under the contract BG051PO001-3.3.06-0047. The authors thank the Director of Skinakas Observatory Prof. I. Pa

Results from UBVRI optical photometric observations of the pre-main sequence star V350 Cep during the period 2004-2014 are presented.The star was discovered in 1977 due to its remarkable increase in brightness by more than 5 mag(R).In previous studies,V35