The Formation of Massive Stars: from Herschel to Near-Infrared
| dc.contributor.author | Persi, Paolo | |
| dc.contributor.author | Tapia, Mauricio | |
| dc.date.accessioned | 2023-01-18T14:10:33Z | |
| dc.date.available | 2023-01-18T14:10:33Z | |
| dc.date.issued | 2014 | |
| dc.identifier.citation | Acta Polytechnica. 2014, vol. 1, no. 1, p. 103-107. | |
| dc.identifier.issn | 1210-2709 (print) | |
| dc.identifier.issn | 1805-2363 (online) | |
| dc.identifier.uri | http://hdl.handle.net/10467/105698 | |
| dc.description.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 μm) 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 H2 and Kc narrow-band images, we have found an H2 jet in this region. | en |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | eng | |
| dc.publisher | České vysoké učení technické v Praze | cs |
| dc.publisher | Czech Technical University in Prague | en |
| dc.relation.ispartofseries | Acta Polytechnica | |
| dc.relation.uri | https://ojs.cvut.cz/ojs/index.php/APP/article/view/2355 | |
| dc.rights | Creative Commons Attribution 4.0 International License | en |
| dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | |
| dc.title | The Formation of Massive Stars: from Herschel to Near-Infrared | |
| dc.type | article | en |
| dc.date.updated | 2023-01-18T14:10:33Z | |
| dc.identifier.doi | 10.14311/APP.2014.01.0103 | |
| dc.rights.access | openAccess | |
| dc.type.status | Peer-reviewed | |
| dc.type.version | publishedVersion |
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