Counter images in closed elliptical friedmann universes

dc.contributor.authorNarlikar, J. V.
dc.contributor.authorSeshadri, T. R.
dc.date.accessioned2012-03-25T09:52:52Z
dc.date.available2012-03-25T09:52:52Z
dc.date.issued1985-01-06
dc.description.abstractIt is shown that the different connectivity implied by the elliptical version of a closed Friedmann model allows two images of a distant astronomical object to be seen, provided the deceleration parameter q0 of the Friedmann model exceeds unity. Of the two images the direct image is along the shortest-route light track. If the redshift of the direct image exceeds (1.5q0 - 1)/(q0 - 1)sq then a second counterimage should be visible at the diametrically antipodal position. The direct image has a maximum possible redshift, and it is suggested that the apparent cutoff in the redshifts of QSOs may be due to this effect. Other observable consequences of this result are discussed in relation to galaxies and QSOs.en_US
dc.identifier.urihttp://hdl.handle.net/11007/1606
dc.language.isoenen_US
dc.publisherAmerican Astronomical Societyen_US
dc.relation.ispartofseriesThe Astrophysical Journal;Vol. 288, 1985
dc.subjectAstronomical modelsen_US
dc.subjectCosmologyen_US
dc.subjectUniverseen_US
dc.subjectDecelerationen_US
dc.subjectMagnitudeen_US
dc.subjectQuasarsen_US
dc.subjectRed shiften_US
dc.titleCounter images in closed elliptical friedmann universesen_US
dc.typeArticleen_US

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