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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6904
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dc.contributor.authorShastri, P-
dc.contributor.authorGomez, E. J-
dc.contributor.authorGupta, M-
dc.contributor.authorMadejski, G-
dc.date.accessioned2020-11-11T01:47:11Z-
dc.date.available2020-11-11T01:47:11Z-
dc.date.issued2015-03-
dc.identifier.citationProceedings of the International Astronomical Union, Vol. 313, pp. 164-168en_US
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/6904-
dc.descriptionRestricted Access © Cambridge University Press http://dx.doi.org/10.1017/S1743921315002124en_US
dc.description.abstractWe investigate the systematics of the properties of highly relativistic jets at multiple frequencies, including Fermi, and MOJAVE data. We test the hypothesis that the blazar divide constitutes a dichotomy. We also explore possible measures of the Doppler factor for these highly Doppler-beamed active galactic nuclei.en_US
dc.language.isoenen_US
dc.publisherCambridge University Pressen_US
dc.subjectGalaxies :activeen_US
dc.subjectGalaxies: jetsen_US
dc.titleSystematics of jets using multi-wavelength dataen_US
dc.typeArticleen_US
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