http://arxiv.org/abs/1802.07996
Results from BVRI 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.
S. Ibryamov, E. Semkov, S. Peneva, et. al.
Fri, 23 Feb 18
35/64
Comments: Accepted for publication in BAJ