A long-term photometric study of the FU Orionis star V 733 Cep

TL;DR

This study presents a long-term photometric analysis of the FU Orionis star V 733 Cep, combining new CCD data with archival photographic plates to understand its variability and stellar evolution.

Contribution

It provides the first extensive long-term light curve of V 733 Cep, integrating CCD and archival data to analyze its photometric behavior over several years.

Findings

Constructed a historical light curve of V 733 Cep.

Identified photometric variability patterns in the star.

Calibrated comparison stars for accurate photometry.

Abstract

The FU Orionis candidate V733 Cep was discovered by Roger Persson in 2004. The star is located in the dark cloud L1216 close to the Cepheus OB3 association. Because only a small number of FU Orionis stars have been detected to date, photometric and spectral studies of V733 Cep are of great interest. The studies of the photometrical variability of PMS stars are very important to the understanding of stellar evolution. The main purpose of our study is to construct a long-time light curve of V733 Cep. On the basis of BVRI monitoring we also study the photometric behavior of the star. We gather data from CCD photometry and archival photographic plates. The photometric BVRI data (Johnson-Cousins system) that we present were collected from June 2008 to October 2009. To facilitate transformation from instrumental measurements to the standard system, fifteen comparison stars in the field of V733 Cep were calibrated in BVRI bands. To construct a historical light curve of V733 Cep, a search for archival photographic observations in the Wide-Field Plate Database was performed. As a result, 192 photographic plates containing the field of V733 Cep were found. Some plates were analyzed at our request to estimate the magnitude of V733 Cep.