Non-variable 13.5 mm flux in the strong millimetre component of Centaurus A

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dc.contributor.authorFogarty W.G.
dc.contributor.authorSchuch N.J.
dc.date.accessioned2024-03-13T01:47:57Z
dc.date.available2024-03-13T01:47:57Z
dc.date.issued1975
dc.description.abstractIT has been suggested1 that the peculiar galaxy and strong radio source Cen A has a strong and possibly variable component in the millimetre wavelength region. © 1975 Nature Publishing Group.
dc.description.firstpage124
dc.description.issuenumber5496
dc.description.lastpage125
dc.description.volume254
dc.identifier.doi10.1038/254124a0
dc.identifier.issn0028-0836
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/38090
dc.relation.ispartofNature
dc.rightsAcesso Restrito
dc.titleNon-variable 13.5 mm flux in the strong millimetre component of Centaurus A
dc.typeCarta ao editor
local.scopus.citations5
local.scopus.eid2-s2.0-0346475515
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=0346475515&origin=inward
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