Subir material

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

 

Mostrar el registro sencillo del ítem

dc.date.accessioned 2022-08-05T19:22:04Z
dc.date.available 2022-08-05T19:22:04Z
dc.date.issued 1976
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/140070
dc.description.abstract An object located approximately atl=8°,b=−4° with a mean radial velocity of −212.3 km s−1 has been observed in the 21 cm neutral hydrogen line. The mean weighted velocity dispersion is 11.2 km s−1 and the total mass is estimated to be 190R2 (kpc) solar masses. We discuss possible interpretations of the origin and nature of this object. The most likely interpretation is that we observe an expanding object which has been ejected from the galactic nucleus. en
dc.format.extent 483-494 es
dc.language en es
dc.subject Hydrogen es
dc.subject Total Mass es
dc.subject High Velocity es
dc.subject Radial Velocity es
dc.subject Velocity Dispersion es
dc.title An expanding high velocity hi cloud probably ejected from the galactic nucleus en
dc.type Articulo es
sedici.identifier.other doi:10.1007/bf01225972 es
sedici.identifier.issn 0004-640x es
sedici.identifier.issn 1572-946x es
sedici.creator.person Mirabel Miquele, Igor Félix es
sedici.creator.person Franco, M. L. es
sedici.subject.materias Ciencias Exactas 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 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. 42, no. 2 es


Descargar archivos

Thumbnail
Documento
Descargar archivo (528.9Kb) - PDF

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

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)