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Long-term photometric behavior of the PMS stars V977 Cep and V982 Cep in the vicinity of NGC 7129
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作者 Sunay I. Ibryamov evgeni h. semkov +1 位作者 Teodor R. Milanov Stoyanka P. Peneva 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2017年第2期77-88,共12页
Long-term BVRI photometric light curves of the pre-main sequence stars V977 Cep and V982 Cep during the period from 2000 October to 2016 August are presented. The stars are located in the vicinity of the reflection ne... Long-term BVRI photometric light curves of the pre-main sequence stars V977 Cep and V982 Cep during the period from 2000 October to 2016 August are presented. The stars are located in the vicinity of the reflection nebula NGC 7129. Our photometric data show that both stars exhibit strong photometric variability in all optical passbands, which is typical for Classical T Tauri stars. Using our observational data we analyze the reasons for the observed brightness variations. In the case of V977 Cep we identify previously unknown periodicity in its light curve. 展开更多
关键词 stars: pre-main sequence -- variables: T Tauri -- stars: individual (V977 Cep V982 Cep)
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