Expanding HI in the Car OB2

dc.creatorRizzo, José Ricardo
dc.creatorArnal, Edmundo Marcelo
dc.creatorBajaja, Esteban
dc.date1990
dc.date2022-09-26T12:43:24Z
dc.date.accessioned2023-07-15T08:14:34Z
dc.date.available2023-07-15T08:14:34Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/142703
dc.identifierissn:1669-9521
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7483562
dc.descriptionFrom the analysis of the interstellar HI in the region of Car OB2, it was possible to identify a large structure, presumably related to the association. This structure, immersed in a very complex ambient (it is seen throughout the Sagitario-Carina arm), consists of a shell expanding at 24 km s¯¹, and of a bubble located in the central part. The coincidences in position, velocity and age strengthen the relationship between Car OB2 and this structure , created by the effect of the evolution of its most massive stars on the interstellar medium.
dc.descriptionAsociación Argentina de Astronomía
dc.formatapplication/pdf
dc.languagees
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectAstronomía
dc.subjectGalaxia
dc.subjectcar ob2
dc.titleExpanding HI in the Car OB2
dc.typeArticulo
dc.typeComunicacion


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