22.2-GHz high emission nebulosities associated with the Carina Nebula central region

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dc.contributor.authorScalise Jr. E.
dc.contributor.authorKaufmann P.
dc.contributor.authorAlcina Braz M.
dc.date.accessioned2024-03-13T01:48:05Z
dc.date.available2024-03-13T01:48:05Z
dc.date.issued1974
dc.description.abstractMAPS of Carina Nebula, obtained at relatively low frequencies, have shown that most of the radiation arises from a central region and has a simple double structure, separated by about 9.4′. Gardner et al.1 studied Carina Nebula at 5 GHz, the highest frequency so far used, with the Parkes radio telescope and observed a beamwidth of 4′. © 1974 Nature Publishing Group.
dc.description.firstpage663
dc.description.issuenumber5485
dc.description.lastpage664
dc.description.volume252
dc.identifier.doi10.1038/252663a0
dc.identifier.issn0028-0836
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38098
dc.relation.ispartofNature
dc.rightsAcesso Restrito
dc.title22.2-GHz high emission nebulosities associated with the Carina Nebula central region
dc.typeArtigo
local.scopus.citations2
local.scopus.eid2-s2.0-36949053510
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=36949053510&origin=inward
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