Subir material

Suba sus trabajos a SEDICI, para mejorar notoriamente su visibilidad e impacto

 

Mostrar el registro sencillo del ítem

dc.date.accessioned 2022-06-07T14:52:21Z
dc.date.available 2022-06-07T14:52:21Z
dc.date.issued 1980
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/137469
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. en
dc.format.extent 247-248 es
dc.language en es
dc.title A search for HI in nine southern galactic clusters en
dc.type Articulo es
sedici.identifier.other doi:10.1017/s007418090009197x es
sedici.identifier.issn 0074-1809 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.description.fulltext true es
mods.originInfo.place Instituto Argentino de Radioastronomía 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 Symposium - International Astronomical Union es
sedici.relation.journalVolumeAndIssue vol. 85 es


Descargar archivos

Thumbnail
Documento
Descargar archivo (453.4Kb) - PDF

Este ítem aparece en la(s) siguiente(s) colección(ones)

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)