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Acta Polytechnica CTU Proceedings, 1(1), p. 103-107, 2014

DOI: 10.14311/app.2014.01.0103

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The Formation of Massive Stars: from Herschel to Near-Infrared

Journal article published in 2014 by Paolo Persi, Mauricio Tapia ORCID
This paper was not found in any repository; the policy of its publisher is unknown or unclear.
This paper was not found in any repository; the policy of its publisher is unknown or unclear.

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Abstract

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.

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