A multi-wavelength analysis of the diffuse HII region G25.8700+0.1350
We present a multi-wavelength investigation of the H II region G25.8700+0.1350, located in the inner part of the Galaxy. In radio continuum emission, the region is seen as a bright arcshaped structure. An analysis of the H I line suggests that G25.8700+0.1350 lies at a distance of 6.5 kpc. The ioniz...
Guardado en:
Autores principales: | , , , , |
---|---|
Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00358711_v474_n1_p647_Cichowolski |
Aporte de: |
id |
todo:paper_00358711_v474_n1_p647_Cichowolski |
---|---|
record_format |
dspace |
spelling |
todo:paper_00358711_v474_n1_p647_Cichowolski2023-10-03T14:47:23Z A multi-wavelength analysis of the diffuse HII region G25.8700+0.1350 Cichowolski, S. Duronea, N.U. Suad, L.A. Reynoso, E.M. Dorda, R. H II regions Infrared: ISM ISM: bubbles Stars: formation Stars: massive We present a multi-wavelength investigation of the H II region G25.8700+0.1350, located in the inner part of the Galaxy. In radio continuum emission, the region is seen as a bright arcshaped structure. An analysis of the H I line suggests that G25.8700+0.1350 lies at a distance of 6.5 kpc. The ionized gas is bordered by a photodissociation region, which is encircled by a molecular structure where four molecular clumps are detected. At infrared wavelengths, the region is also very conspicuous. Given the high level of visual absorption in the region, the exciting stars should be searched for in the infrared band. In this context, we found in the literature one Wolf-Rayet and one red supergiant, which, together with 37 2MASS sources that are candidate O-type stars, could be related to the origin of G25.8700+0.1350. Finally, as expanding H II regions are hypothesized to trigger star formation, we used different infrared point source catalogues to search for young stellar object candidates (cYSOs). A total of 45 cYSOs were identified projected on to the molecular clouds. © 2017 The Authors. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00358711_v474_n1_p647_Cichowolski |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
H II regions Infrared: ISM ISM: bubbles Stars: formation Stars: massive |
spellingShingle |
H II regions Infrared: ISM ISM: bubbles Stars: formation Stars: massive Cichowolski, S. Duronea, N.U. Suad, L.A. Reynoso, E.M. Dorda, R. A multi-wavelength analysis of the diffuse HII region G25.8700+0.1350 |
topic_facet |
H II regions Infrared: ISM ISM: bubbles Stars: formation Stars: massive |
description |
We present a multi-wavelength investigation of the H II region G25.8700+0.1350, located in the inner part of the Galaxy. In radio continuum emission, the region is seen as a bright arcshaped structure. An analysis of the H I line suggests that G25.8700+0.1350 lies at a distance of 6.5 kpc. The ionized gas is bordered by a photodissociation region, which is encircled by a molecular structure where four molecular clumps are detected. At infrared wavelengths, the region is also very conspicuous. Given the high level of visual absorption in the region, the exciting stars should be searched for in the infrared band. In this context, we found in the literature one Wolf-Rayet and one red supergiant, which, together with 37 2MASS sources that are candidate O-type stars, could be related to the origin of G25.8700+0.1350. Finally, as expanding H II regions are hypothesized to trigger star formation, we used different infrared point source catalogues to search for young stellar object candidates (cYSOs). A total of 45 cYSOs were identified projected on to the molecular clouds. © 2017 The Authors. |
format |
JOUR |
author |
Cichowolski, S. Duronea, N.U. Suad, L.A. Reynoso, E.M. Dorda, R. |
author_facet |
Cichowolski, S. Duronea, N.U. Suad, L.A. Reynoso, E.M. Dorda, R. |
author_sort |
Cichowolski, S. |
title |
A multi-wavelength analysis of the diffuse HII region G25.8700+0.1350 |
title_short |
A multi-wavelength analysis of the diffuse HII region G25.8700+0.1350 |
title_full |
A multi-wavelength analysis of the diffuse HII region G25.8700+0.1350 |
title_fullStr |
A multi-wavelength analysis of the diffuse HII region G25.8700+0.1350 |
title_full_unstemmed |
A multi-wavelength analysis of the diffuse HII region G25.8700+0.1350 |
title_sort |
multi-wavelength analysis of the diffuse hii region g25.8700+0.1350 |
url |
http://hdl.handle.net/20.500.12110/paper_00358711_v474_n1_p647_Cichowolski |
work_keys_str_mv |
AT cichowolskis amultiwavelengthanalysisofthediffusehiiregiong25870001350 AT duroneanu amultiwavelengthanalysisofthediffusehiiregiong25870001350 AT suadla amultiwavelengthanalysisofthediffusehiiregiong25870001350 AT reynosoem amultiwavelengthanalysisofthediffusehiiregiong25870001350 AT dordar amultiwavelengthanalysisofthediffusehiiregiong25870001350 AT cichowolskis multiwavelengthanalysisofthediffusehiiregiong25870001350 AT duroneanu multiwavelengthanalysisofthediffusehiiregiong25870001350 AT suadla multiwavelengthanalysisofthediffusehiiregiong25870001350 AT reynosoem multiwavelengthanalysisofthediffusehiiregiong25870001350 AT dordar multiwavelengthanalysisofthediffusehiiregiong25870001350 |
_version_ |
1782028908002017280 |