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dc.date.accessioned 2020-05-06T11:59:55Z
dc.date.available 2020-05-06T11:59:55Z
dc.date.issued 1969
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/95041
dc.description.abstract The distribution and motions of both neutral and ionized hydrogen can be studied throughout the Galaxy by radio methods. The neutral hydrogen is observed through the 21-cm hyperfine transition line; the continuity of many prominent features indicates that we are seeing the galactic spiral pattern, but it is difficult to locate the spiral arms in space because we are restricted to kinematic distance estimates for the hydrogen. es
dc.language es es
dc.subject Galaxias es
dc.title Some problems associated with large scale galactic structure en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Kerr, F. 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. 14 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)