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ИСТИНА ПсковГУ |
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We provide infrared photometric monitoring of young stellar objects in vicinity of variable water or/and class II methanol maser sources. The observations are conducted with the instruments of the Sternberg Astronomical Institute (Lomonosov Moscow University). As first results of monitoring, we observed the variation of G025.65+1.05 and G107.298+5.639 K-band emission during maser flares in comparison with archive data.