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.
@article{arxiv.1802.07996,
title = {Multicolor photometric behavior of the young stellar object V1704 Cygni},
author = {Sunay Ibryamov and Evgeni Semkov and Stoyanka Peneva and Ugur Karadeniz},
journal= {arXiv preprint arXiv:1802.07996},
year = {2018}
}