Photometric monitoring of Luminous Blue Variables
INAF-Osservatorio Astrofisico di Catania, Catania Italy
INAF-Osservatorio Astrofisico di Catania, Catania Italy, and Dipartimento di Fisica e Astronomia, Universitá di Catania, Catania Italy
INAF-Osservatorio Astrofisico di Catania, Catania Italy
INAF- Istituto di Radioastronomia, Noto, Italy
INAF-Osservatorio Astrofisico di Catania, Catania Italy
INAF-Osservatorio Astrofisico di Catania, Catania Italy
Osservatorio astronomico, Bologna,Italy
INAF-Osservatorio Astrofisico di Catania, Catania Italy
INAF-Osservatorio Astrofisico di Catania, Catania Italy
Abstract
We present some preliminary results from our program of intensive near-infrared photometric monitoring of a sample of confirmed and candidate Luminous Blue Variables (LBVs) conducted from 2008 to 2010.
Clear long-term variability has been observed for Wray 17-96 and V481 Sct, with overall brightness variation greater than 1 mag in the J band. Other sources, such as LBV 1806-20 showed detectable variability with amplitudes of few tenths of a magnitude with a time-scale of about 60 days.