- Startpagina tijdschrift
- Volume 80 - Année 2011
- Photometric monitoring of Luminous Blue Variables
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Photometric monitoring of Luminous Blue Variables
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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.
Om dit artikel te citeren:
Over : Carla Buemi
INAF-Osservatorio Astrofisico di Catania, Catania Italy
Over : Elisa Distefano
INAF-Osservatorio Astrofisico di Catania, Catania Italy, and Dipartimento di Fisica e Astronomia, Universitá di Catania, Catania Italy
Over : Paolo Leto
INAF-Osservatorio Astrofisico di Catania, Catania Italy
Over : Francesco Schillirò
INAF- Istituto di Radioastronomia, Noto, Italy
Over : Corrado Trigilio
INAF-Osservatorio Astrofisico di Catania, Catania Italy
Over : Grazia Umana
INAF-Osservatorio Astrofisico di Catania, Catania Italy
Over : Stefano Bernabei
Osservatorio astronomico, Bologna,Italy
Over : Giuseppe Cutispoto
INAF-Osservatorio Astrofisico di Catania, Catania Italy
Over : Sergio Messina
INAF-Osservatorio Astrofisico di Catania, Catania Italy