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Dark spots, bubbles, and shells in the lobes of extragalactic radio sources

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dc.contributor.authorKundt, W.
dc.contributor.authorSaripalli, Lakshmi
dc.date.accessioned2012-07-14T10:23:39Z
dc.date.available2012-07-14T10:23:39Z
dc.date.issued1987
dc.descriptionOpen Accessen
dc.description.abstractBased on maps of the extragalactic radio sources Cyg A, Her A, Cen A, 3C 277.3 and others, arguments are given that the twin-jets from the respective active galactic nucleus ram their channels repeatedly through thin, massive shells. The jets are thereby temporarily choked and blow radio bubbles. Warm shell matter in the cocoon shows up radio-dark through electron-scattering.en
dc.identifier.citationJournal of Astrophysics and Astronomy, 1987, Vol.8, p211en
dc.identifier.issn0250-6335
dc.identifier.issn0973-7758 (Online)
dc.identifier.urihttp://hdl.handle.net/2289/4934
dc.language.isoenen
dc.publisherIndian Academy of Sciences, Bangalore, Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1987JApA....8..211Ken
dc.relation.urihttp://dx.doi.org/10.1007/BF02715042en
dc.rights1989 Indian Academy of Sciences, Bangalore, Indiaen
dc.subjectextragalactic radio sourcesen
dc.subjectgalactic nucleien
dc.subjectgalactic structureen
dc.subjectradio jets (astronomy)en
dc.subjectspatial distributionen
dc.subjectactive galactic nucleien
dc.subjectbrightness distributionen
dc.subjectbubblesen
dc.titleDark spots, bubbles, and shells in the lobes of extragalactic radio sourcesen
dc.typeArticleen

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