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:
| Publicado: |
2018
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v474_n1_p647_Cichowolski http://hdl.handle.net/20.500.12110/paper_00358711_v474_n1_p647_Cichowolski |
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