Multicolor photometric behavior of the young stellar object V1704 Cygni
Sunay Ibryamov, Evgeni Semkov, Stoyanka Peneva, Ugur Karadeniz
TL;DR
This study presents multi-year BVRI photometric observations of the young star V1704 Cyg, revealing its variability and classification as a classical T Tauri star within the star-forming region IC 5070.
Contribution
It provides detailed long-term photometric data and confirms the star's classification, contributing to understanding of young stellar object behaviors.
Findings
V1704 Cyg exhibits variability in all optical passbands.
The star is classified as a classical T Tauri star.
Photometric data collected over 7 years.
Abstract
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.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsStellar, planetary, and galactic studies · Astrophysics and Star Formation Studies · Astronomical Observations and Instrumentation