Multicolor Photometric Behavior of the Young Stellar Object V1704 Cygni
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Abstract
Results from BV RI photometric observations of the pre-main sequence star V1704 Cyg collected during the time period from August 2010 to December 2017 are presented. The star is located in the star-forming HII region IC 5070 and it exhibits photometric variability in all optical passbands. After analyzing the obtained data, V1704 Cyg is classified as a classical T Tauri star.
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Stars: pre-main sequence, Stars: variables: T Tauri, Star: individual: (V1704 Cyg)
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Volume
29
Issue
Start Page
10
End Page
18
