Subir material

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

 

Mostrar el registro sencillo del ítem

dc.date.accessioned 2020-05-08T13:03:05Z
dc.date.available 2020-05-08T13:03:05Z
dc.date.issued 1969
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/95381
dc.description.abstract The high-velocity hydrogen clouds at high latitudes have been widely discussed as material falling into the galactic disk from outside. The observed velocities show strong effects arising from the galactic rotation at the Sun's position. When this rotation is removed, the residual velocities are compatible with the clouds being in highly eccentric orbits around the Galaxy at distances of the order of 50 kpc. We propose new observations which may help to decide between galactic and extra-galactic interpretations. es
dc.language es es
dc.subject Galaxias es
dc.title The high velocity hydrogen clouds considered as satellites of the galaxy 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


Descargar archivos

Thumbnail
Resumen (1 p.)
Descargar archivo (67.21Kb) - 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)