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Issue DateTitleAuthor(s)Citation
Jan-1981The Maximum Entropy Method of Image Restoration Properties and LimitationsKomesaroff, M.M.; Narayan, R.; Nityananda, R.Astronomy and Astrophysics, 1981, Vol.93, p269-281.
Oct-1981Observations and interpretation of the slowly varying component of solar radio emission at decameter wavelengthsSastry, Ch.V.; Dwarakanath, K.S.; Shevgaonkar, R.K.; Krishan, VinodSolar Physics, 1981, Vol.73, p363-377
1984The relevance of the Eddington limit to thick accretion disksNityananda, R.; Narayan, R.Advances in Space Research, 1984, Vol.3, p319-321
1981The pulsar magnetic windowShukre, C.S.; Radhakrishnan, V.IAU Symposium, 1981, Vol.95, p103
Sep-1983Observations on the slowly varying component of solar radio emission at decameter wavelengthsSastry, Ch.V.; Shevgaonkar, R.K.; Ramanuja, M.N.Solar Physics, 1983, Vol.87, p391-399
1981Polar CAP relief and integrated pulse structureVivekanand, M.; Radhakrishnan, V.IAU Symposium, 1981, Vol.95, p173
1983On the association between pulsars and supernova remnantsRadhakrishnan, V.; Srinivasan, G.IAU Symposium, 1983, Vol.101, p487-494
1989A search for radio recombination lines of positronium near the galactic centerAnantharamaiah, K.R.; Radhakrishnan, V.; Morris, D.; Vivekanand, M.; Downes, D.; Shukre, C.S.IAU Symposium, 1989, Vol.136, p607
1989A survey of radio recombination line emission from the galactic center regionAnantharamaiah, K.R.; Yusef-Zadeh, F.IAU Symposium, 1989, Vol.136, p159
1981Pulsar activity and supernova remnant morphologyRadhakrishnan, V.; Srinivasan, G.IAU Symposium, 1981, Vol.95, p417