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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 1.

VPHAS g-band image of M17, overlaid with 850 μm dust continuum contours (in levels 0.3, 0.6, 1.8, 3.6, 6.0, 9.0, 1.26, and 1.68 Jy beam−1) from JCMT-SCUBA2. The optically bright nebula in M17 is labeled as the M17 H II region, while the northern and southwestern clouds are labeled as M17 North and M17 SW, respectively.

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