2020
DOI: 10.52526/25792776-2020.67.2-187
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Properties of ISM in two star-forming regions

Abstract: The Hi-GAL provides an opportunity to make a complete and unbiased view of the continuum emission in the Galactic plane in five bands: 70, 160, 250, 350, and 500 μm. Our research focuses on two of star-forming regions. The first one is the molecular cloud, which includes G45.12+0.13 and G45.07+0.13 UCHII regions. Using the Modified blackbody fitting on Herschel images obtained in four bands: 160, 250, 350, and 500 μm, we determined the distribution of N(H2) hydrogen column density and Td dust temperature. The … Show more

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Cited by 2 publications
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“…For all regions a detailed study was conducted, which includes the following topics: 1) determination of the parameters of ISM, namely the distribution of N(H 2 ) hydrogen column density and T d dust temperature; 2) the search for young stellar clusters; 3) identification of the clusters' members using their infrared properties; 4) investigation of the structural properties of the young stellar clusters; 5) determination of the age and age spread of the clusters' members; 6) construction of the Luminosity Functions and Mass Functions for the clusters. This thesis is based on the papers Azatyan (2019), Azatyan & Nikoghosyan (2018), Azatyan et al (2016Azatyan et al ( , 2020Azatyan et al ( , 2022, Nikoghosyan & Azatyan (2014), Nikoghosyan et al (2020Nikoghosyan et al ( , 2021.…”
Section: Introductionmentioning
confidence: 99%
“…For all regions a detailed study was conducted, which includes the following topics: 1) determination of the parameters of ISM, namely the distribution of N(H 2 ) hydrogen column density and T d dust temperature; 2) the search for young stellar clusters; 3) identification of the clusters' members using their infrared properties; 4) investigation of the structural properties of the young stellar clusters; 5) determination of the age and age spread of the clusters' members; 6) construction of the Luminosity Functions and Mass Functions for the clusters. This thesis is based on the papers Azatyan (2019), Azatyan & Nikoghosyan (2018), Azatyan et al (2016Azatyan et al ( , 2020Azatyan et al ( , 2022, Nikoghosyan & Azatyan (2014), Nikoghosyan et al (2020Nikoghosyan et al ( , 2021.…”
Section: Introductionmentioning
confidence: 99%