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dc.date.accessioned 2022-06-23T15:24:45Z
dc.date.available 2022-06-23T15:24:45Z
dc.date.issued 1979
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/138243
dc.description.abstract The results of a search for H I features in nine galactic clusters are reported. In six of the clusters the earliest spectral types represented are in the range B0–B9. On the whole, twelve H I features (nine maxima and three minima) were detected, of which seven were disregarded as they were not related to any cluster. The conclusion is that at least in six clusters (Cr 121, Cr 140, Cr 132a, b, Ru 3 and Ru 106) no related H I could be detected. For the remainder (NGC 5460, Cr 135 and Cr 394), the evidence was inconclusive. Our results are in agreement with the qualitative conclusion from earlier work that interstellar H I should be expected only in relatively young clusters. es
dc.format.extent 353-368 es
dc.language en es
dc.subject galactic clusters es
dc.subject interstellar H I es
dc.title A search for H I in nine southern galactic clusters es
dc.type Articulo es
sedici.identifier.other doi:10.1007/bf00650010 es
sedici.identifier.issn 0004-640x es
sedici.identifier.issn 1572-946x es
sedici.creator.person Olano, Carlos Alberto es
sedici.creator.person Pöppel, Wolfgang G. L. es
sedici.creator.person Vota, M. D. es
sedici.subject.materias Astronomía es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Universidad Nacional de La Plata es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution 4.0 International (CC BY 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Astrophysics and Space Science es
sedici.relation.journalVolumeAndIssue vol. 66, no. 2 es


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