Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6937
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dc.contributor.authorNandi, S-
dc.contributor.authorSaikia, D. J-
dc.contributor.authorRoy, R-
dc.contributor.authorDabhade, P.-
dc.contributor.authorWadadekar, Y-
dc.contributor.authorLarsson, J-
dc.contributor.authorBaes, M-
dc.contributor.authorChandola, H. C-
dc.contributor.authorSingh, M-
dc.date.accessioned2020-11-12T14:51:23Z-
dc.date.available2020-11-12T14:51:23Z-
dc.date.issued2019-07-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 486, No. 4, pp. 5158-5170en_US
dc.identifier.issn0035-8711-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/6937-
dc.descriptionRestricted Access © Royal Astronomical Society https://doi.org/10.1093/mnras/stz1184en_US
dc.description.abstractn order to understand the possible mechanisms of recurrent jet activity in radio galaxies and quasars, which are still unclear, we have identified such sources with a large range of linear sizes (220–917 kpc), and hence timescales of episodic activity. Here we present high-sensitivity 607-MHz Giant Metrewave Radio Telescope (GMRT) images of 21 possible double-double radio galaxies (DDRGs) identified from the FIRST survey to confirm their episodic nature. These GMRT observations show that none of the inner compact components suspected to be hotspots of the inner doubles are cores having a flat radio spectrum, confirming the episodic nature of these radio sources. We have identified a new DDRG with a candidate quasar, and have estimated the upper spectral age limits for eight sources which showed marginal evidence of steepening at higher frequencies. The estimated age limits (11–52 Myr) are smaller than those of the large-sized ( ∼ 1 Mpc) DDRGs.en_US
dc.language.isoenen_US
dc.publisherOxford University Press on behalf of the Royal Astronomical Societyen_US
dc.subjectgalaxiesen_US
dc.subjectactive – galaxiesen_US
dc.subjectevolution – galaxiesen_US
dc.subjectjets – galaxiesen_US
dc.subjectnuclei – (galaxies:) quasarsen_US
dc.subjectupermassive black holesen_US
dc.subjectradio continuum: galaxiesen_US
dc.titleA Low-Frequency Study of Recently Identified Double-Double Radio Galaxiesen_US
dc.typeArticleen_US
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