Long-term optical photometric monitoring of the FUor star V900 Mon
Evgeni Semkov, Stoyanka Peneva, Sunay Ibryamov

TL;DR
This study presents a decade-long optical photometric monitoring of V900 Mon, revealing a gradual brightness increase since 2011, with an outburst amplitude of about 4 magnitudes, contributing valuable data on FUor star variability.
Contribution
First long-term optical photometric study of V900 Mon, providing detailed light curve analysis and comparison with other FUor stars, enhancing understanding of FUor outburst behaviors.
Findings
Brightness increased gradually from 2011 to 2017
Outburst amplitude is approximately 4 magnitudes
Light curve resembles V1515 Cyg and V733 Cep
Abstract
We present results from photometric monitoring of V900 Mon, one of the newly discovered and still under-studied object from FU Orionis type. FUor phenomenon is very rarely observed, but it is essential for stellar evolution. Since we only know about twenty stars of this type, the study of each new object is very important for our knowledge. Our data was obtained in the optical spectral region with BVRI Johnson-Cousins set of filters during the period from September 2011 to April 2021. In order to follow the photometric history of the object, we measured its stellar magnitudes on the available plates from the Mikulski Archive for Space Telescopes. The collected archival data suggests that the rise in brightness of V900 Mon began after January 1989 and the outburst goes so far. In November 2009, when the outburst was registered, the star had already reached a level of brightness close to…
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.
