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Periodic flare of the 6.7-GHz methanol maser in IRAS22198+6336

机译:IRAS22198 + 6336中6.7 GHz甲醇maser的周期性耀斑

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We have detected periodic flares of the 6.7-GHz methanol maser from an intermediatemass star-forming region IRAS 22198+6336. The maser was monitored daily in 2011, 2012, and 2013. Six flares were observed with a period of 34.6 d. The variation pattern is intermittent, and the flux ratio of the flaring and the quiescent states exceeds 30. Such intermittent variation with the short period uniquely characterizes the variation of the IRAS 22198+6336 maser. At least five spectral components were identified. The spectral components varied almost synchronously, but their peak times differed by 1.8 d. These characteristics can be explained by the colliding-wind binary model.
机译:我们已经从一个中等质量恒星形成区域IRAS 22198 + 6336中检测到6.7 GHz甲醇maser的周期性耀斑。分别在2011年,2012年和2013年对微波激射器进行了监测。观测到了6个耀斑,持续时间为34.6 d。变化模式是间歇性的,扩口和静止状态的通量比超过30。这种具有短周期的间歇性变化是IRAS 22198 + 6336 maser的独特变化。至少鉴定出五个光谱成分。光谱成分几乎同步变化,但其峰值时间相差1.8 d。这些特征可以通过碰撞风二进制模型来解释。

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