The Formation of Massive Stars: from Herschel to Near-Infrared
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We have studied a number of selected high mass star forming regions, including high resolution near-infrared broad- and narrow-band imaging, Herschel (70, 160, 250, 350 and 500<em> μ</em>m) and Spitzer (3.6, 4.5, 5.8 and 8.0 m) images. The preliminary results of one of this region, IRAS 19388+2357(MOL110) are discussed. In this region a dense core has been detected in the far-infrared, and a young stellar cluster has been found around this core. Combining near-IR data with Spitzer and Herschel photometry we have derived the spectral energy distribution of Mol110. Finally comparing our H<sub>2</sub> and Kc narrow-band images, we have found an H<sub>2</sub> jet in this region.
2020 ◽
Vol 496
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pp. 3358-3370
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2018 ◽
Vol 615
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pp. A146
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2001 ◽
Vol 205
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pp. 284-285
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2020 ◽
pp. 241-250
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1997 ◽
Vol 163
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pp. 725-726
Nitrogen and hydrogen fractionation in high-mass star-forming cores from observations of HCN and HNC
2018 ◽
Vol 609
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pp. A129
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