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dc.date.accessioned 2021-01-28T12:13:17Z
dc.date.available 2021-01-28T12:13:17Z
dc.date.issued 1984
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/111827
dc.description.abstract The distribution of neutral hydrogen is studied in the region defined by eq. (1). After subtracting a broad Gaussian component, which could be interpreted as the emission of a hot inter-cloud medium, a Gaussian analysis of the residual 21-cm profiles was performed. The resultant components, of small velocity dispersion, have counterparts in interstellar absorption lines of Na I and Ca II. They could have originated by an expanding phenomenon (like a supernova explosion) produced within the gas related to feature A of Lindblad by stars of the association Sco OB2. As the paper will be published elsewhere, we give here only a synthesis. en
dc.format.extent 40-48 es
dc.language es es
dc.subject Galaxias es
dc.subject Sco OB2 es
dc.title HI y HII en Scorpius-Ophiuchus es
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Cappa, Cristina Elisabet es
sedici.creator.person Pöppel, Wolfgang G. L. es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 28 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)