Long-term BVRI photometry of V1704 Cygni

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 analysing the obtained data, V1704 Cyg is classified as a classical T Tauri star.

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/other/BAJ/29.10
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/BAJ/29.10
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/other/BAJ/29.10
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/other/BAJ/29.10
Provenance
Creator Ibryamov S.; Semkov E.; Peneva S.; Karadeniz U.
Publisher CDS
Publication Year 2019
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy