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SUGIYAMA, KOICHIRO,YONEKURA, YOSHINORI,MOTOGI, KAZUHITO,SAITO, YU,FUJISAWA, KENTA,ISHII, SHOTA,MOMOSE, MUNETAKE,HONMA, MAREKI,TAZAKI, FUMIE,TANAKA, KEI E.I.,HOSOKAWA, TAKASHI,UCHIYAMA, MIZUHO,INAYOSHI The Korean Astronomical Society 2015 天文學論叢 Vol.30 No.2
We have initiated single-dish monitoring observations of ~400 methanol maser sources at 6.7 GHz using the Hitachi 32-m radio telescope from December 2012 to systematically research periodic flux variations, which are observed in some methanol maser sources associated with high-mass (proto-)stars. In our monitoring, we have made daily monitoring, so that each source has been observed every nine days with an integration time of 5 min (typical $3{\sigma}$ detection sensitivities of 0.9 Jy). The monitoring observations help us statistically understand periodic flux variations with a period longer than 50 days. As an initial result, we present a new detection of periodic flux variations in the 6.7 GHz methanol maser source G 036.70+00.09. The period of the flux variations is ~53 days (~0.019 cycles $day^{-1}$), and seems to be stable over 9 cycles, at least until the middle of August 2014.