Photometry and kinematics of extragalactic star-forming complexes

We investigate spectral and photometric properties of extragalactic star-forming complexes (SFCs). The SFCs were selected in 17 nearby galaxies of a spiral or irregular type, having inclinations less than 45° and distances less than 15 Mpc. To identify SFCs, we developed a method based on matching s...

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Main Authors: Kuzin Aleksey, Lisitsin Danil
Format: Article
Language:English
Published: De Gruyter 2022-04-01
Series:Open Astronomy
Subjects:
Online Access:https://doi.org/10.1515/astro-2022-0018
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author Kuzin Aleksey
Lisitsin Danil
author_facet Kuzin Aleksey
Lisitsin Danil
author_sort Kuzin Aleksey
collection DOAJ
description We investigate spectral and photometric properties of extragalactic star-forming complexes (SFCs). The SFCs were selected in 17 nearby galaxies of a spiral or irregular type, having inclinations less than 45° and distances less than 15 Mpc. To identify SFCs, we developed a method based on matching sources of emission at 160μm160\hspace{0.33em}{\rm{\mu }}{\rm{m}} (cold dust) and 8μm8\hspace{0.33em}{\rm{\mu }}{\rm{m}} (polycyclic aromatic hydrocarbons). Using photometry in different spectral bands, correlations between SFC properties for spiral and irregular galaxies were considered. Spectral and kinematic analysis was carried out for several SFCs, and a method to detect gas motion patterns in these SFCs was suggested.
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spelling doaj.art-42f40748777c473392e68a162a920ac62022-12-22T03:33:33ZengDe GruyterOpen Astronomy2543-63762022-04-0131114314710.1515/astro-2022-0018Photometry and kinematics of extragalactic star-forming complexesKuzin Aleksey0Lisitsin Danil1Faculty of Physics, Moscow State University, Moscow, 119991, Russian FederationFaculty of Physics, Moscow State University, Moscow, 119991, Russian FederationWe investigate spectral and photometric properties of extragalactic star-forming complexes (SFCs). The SFCs were selected in 17 nearby galaxies of a spiral or irregular type, having inclinations less than 45° and distances less than 15 Mpc. To identify SFCs, we developed a method based on matching sources of emission at 160μm160\hspace{0.33em}{\rm{\mu }}{\rm{m}} (cold dust) and 8μm8\hspace{0.33em}{\rm{\mu }}{\rm{m}} (polycyclic aromatic hydrocarbons). Using photometry in different spectral bands, correlations between SFC properties for spiral and irregular galaxies were considered. Spectral and kinematic analysis was carried out for several SFCs, and a method to detect gas motion patterns in these SFCs was suggested.https://doi.org/10.1515/astro-2022-0018star formationmolecular cloudsinterstellar medium
spellingShingle Kuzin Aleksey
Lisitsin Danil
Photometry and kinematics of extragalactic star-forming complexes
Open Astronomy
star formation
molecular clouds
interstellar medium
title Photometry and kinematics of extragalactic star-forming complexes
title_full Photometry and kinematics of extragalactic star-forming complexes
title_fullStr Photometry and kinematics of extragalactic star-forming complexes
title_full_unstemmed Photometry and kinematics of extragalactic star-forming complexes
title_short Photometry and kinematics of extragalactic star-forming complexes
title_sort photometry and kinematics of extragalactic star forming complexes
topic star formation
molecular clouds
interstellar medium
url https://doi.org/10.1515/astro-2022-0018
work_keys_str_mv AT kuzinaleksey photometryandkinematicsofextragalacticstarformingcomplexes
AT lisitsindanil photometryandkinematicsofextragalacticstarformingcomplexes