作者: P. Pietrukowicz , D. Minniti , J. Alonso-García , M. Hempel
DOI: 10.1051/0004-6361/201116877
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摘要: We have used deep V-band and JHKs-band observations to investigate variability stellar populations near the Galactic plane in Centaurus, compared with model of Besancon. By applying image subtraction technique a series over 580 frames taken ESO VLT/VIMOS instrument during two contiguous nights April 2005, we detected 333 variables among 84,734 stars brightness range 12.7