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Submillimeter and Mid-infrared Variability of Young Stellar Objects in the M17 H II Region

  • Authors: Zhiwei Chen, 志维 陈, Doug Johnstone, Carlos Contreras Peña, Jeong-Eun Lee, Sheng-Yuan Liu, Gregory Herczeg, 雷歌 沈, Steve Mairs, Geumsook Park, Kee-Tae Kim, Mi-Ryang Kim, Keping Qiu, Yao-Te Wang, Xu Zhang, Megan Reiter

Zhiwei Chen et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 4.

The distribution of the absolute value of the best-fit peak brightness slope S ratioed to its uncertainty ΔS vs. mean peak flux for the 450 (left) and 850 μm (right) sources in M17. The dashed horizontal line in both panels indicates where ∣SS∣ = 3, indicating the threshold for linear variability reliability as defined by D. Johnstone et al. (2018). Bright 450 and 850 μm sources with ∣SS∣ > 3 are highlighted by circles. In the 850 μm plot, only one bright source, JCMTPP J182023.2, has a value of ∣SS∣ much higher than the threshold.

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