http://arxiv.org/abs/1504.06774
Results from long-term multicolor optical photometric observations of the pre-main sequence stars FHO 26, FHO 27, FHO 28, FHO 29 and V1929 Cyg collected during the period from June 1997 to December 2014 are presented. The objects are located in the dense molecular cloud L935, named “Gulf of Mexico”, in the field between the North America and Pelican nebulae. All stars from our study exhibit strong photometric variability in all optical passbands. Using our BVRI observations and data published by other authors, we tried to define the reasons for the observed brightness variations. The presented paper is a part of our long-term photometric study of the young stellar objects in the region of “Gulf of Mexico”.
S. Ibryamov, E. Semkov and S. Peneva
Tue, 28 Apr 15
66/70
Comments: 28 pages, 13 figures, 6 tables, accepted for publication in Publications of the Astronomical Society of Australia (PASA)
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