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dc.date.accessioned 2023-12-05T12:22:20Z
dc.date.available 2023-12-05T12:22:20Z
dc.date.issued 1994
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/161078
dc.description.abstract The study of one of the nine objects classified by Meaburn in 1980 as "Supergiant Bubbles" of the Large Magellanic Cloud has been undertaken by using Hα observations carried out with an imaging Fabry-Pérot interference spectrometer. A morphological, kinematical and photometrical study about this object is here presented, supporting the idea that we are dealing with a spheroidal, expanding shell. The probable origin of this huge superstructure is discussed on the basis of energetic considerations for classic stellar-wind and supernova-explosion models. An alternative approach is also discussed. en
dc.language en es
dc.subject Galaxia es
dc.title The supergiant interstellar bubble LMC 1 en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Goldes, Guillermo es
sedici.creator.person Laval, A. es
sedici.creator.person Carranza, Gustavo José es
sedici.creator.person LeCoarer, E. es
sedici.creator.person Georgelin, Y. P. es
sedici.creator.person Georgelin, Y. M. es
sedici.creator.person Marcelin, M. es
sedici.creator.person Amram, P. es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Comunicacion 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.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 39 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)