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

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4934

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DC Field	Value	Language
dc.contributor.author	Kundt, W.	-
dc.contributor.author	Saripalli, Lakshmi	-
dc.date.accessioned	2012-07-14T10:23:39Z	-
dc.date.available	2012-07-14T10:23:39Z	-
dc.date.issued	1987	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, 1987, Vol.8, p211	en
dc.identifier.issn	0250-6335	-
dc.identifier.issn	0973-7758 (Online)	-
dc.identifier.uri	http://hdl.handle.net/2289/4934	-
dc.description	Open Access	en
dc.description.abstract	Based 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.language.iso	en	en
dc.publisher	Indian Academy of Sciences, Bangalore, India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1987JApA....8..211K	en
dc.relation.uri	http://dx.doi.org/10.1007/BF02715042	en
dc.rights	1989 Indian Academy of Sciences, Bangalore, India	en
dc.subject	extragalactic radio sources	en
dc.subject	galactic nuclei	en
dc.subject	galactic structure	en
dc.subject	radio jets (astronomy)	en
dc.subject	spatial distribution	en
dc.subject	active galactic nuclei	en
dc.subject	brightness distribution	en
dc.subject	bubbles	en
dc.title	Dark spots, bubbles, and shells in the lobes of extragalactic radio sources	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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