|Issue Date||Title||Author(s)||Citation||Dec-1995 ||New HI absorption measurements towards six pulsars||Saravanan, T.P.; Deshpande, A.A.; Srinivasan, G.; McConnell, D.; Wilson, W.; McCulloch, P.M.||Bulletin of the Astronomical Society of India, 1995, Vol.23, p512
||Mar-1982 ||A new look at SNR birthrate and evidence for a predominantly low-density interstellar medium||Srinivasan, G.; Dwarakanath, K.S.||Bulletin of the Astronomical Society of India, 1982, Vol.10, p48
||1982 ||A new look at the birthrate of supernova remnants||Srinivasan, G.; Dwarakanath, K.S.||Journal of Astrophysics and Astronomy, 1982, Vol. 3, p351-361.
||10-Jan-1990 ||A novel mechanism for the decay of neutron star magnetic fields||Srinivasan, G.; Bhattacharya, D.; Muslimov, A.G.; Tsygan, A.J.||Current Science, 1990, Vol. 59, p31-38.
||9-Aug-2009 ||Of stars and singularities||Srinivasan, G.||Radicals in Science: Nature or Nurture?, 9th Aug. 2010
||1985 ||On pulsar - Supernovae remnant associations||Srinivasan, G.||Proceedings of the Academy Workshop on Supernovae, their Progenitors and Remnants, October 29-November 2, 1984, Raman Research Institute, Bangalore. Editors, G. Srinivasan, V. Radhakrishnan; Indian Academy of Sciences, Bangalore, 1985, p105
||1983 ||On the association between pulsars and supernova remnants||Radhakrishnan, V.; Srinivasan, G.||IAU Symposium, 1983, Vol.101, p487-494
||1987 ||On the association between supernova remnants and pulsars||Bhattacharya, D.; Srinivasan, G.||High energy phenomena around collapsed stars; Proceedings of the NATO Advanced Study Institute, Cargese, France, Sept. 2-13, 1985, Dordrecht, D. Reidel Publishing Co., 1987, p235-242
||27-Dec-1973 ||On the electronic contribution to the surface energy of metals||Srinivasan, G.; Jonson, M.||Solid State Communications,1974, Vol.15, p.771
||1995 ||On the fraction of pulsars recycled in binary systems||Deshpande, A.A.; Ramachandran, R.; Srinivasan, G.||Bulletin of the Astronomical Society of India, 1995, Vol.23, p475
||5-Apr-1986 ||On the implication of the recently discovered 5 millisecond binary pulsar PSR 1855+09||Bhattacharya, D.; Srinivasan, G.||Current Science, 1986, Vol. 55, p327-330.
||20-Jun-1982 ||On the implications of the radio and x-ray pulsar in the supernova remnant MSH 15-52||Srinivasan, G.; Dwarakanath, K.S.; Radhakrishnan, V.||Current Science, 1982, Vol. 51, p596-599.
||20-Mar-1989 ||On the implications of the submillisecond pulsar in Supernova 1987A||Bhattacharya, D.; Srinivasan, G.||Current Science, 1989, Vol. 58, p280-286.
||5-Sep-1989 ||On the lifetime of low mass x-ray binaries||Srinivasan, G.; Bhattacharya, D.||Current Science, 1989, Vol. 58, p953-954.
||2001 ||On the limiting mass of neutron stars||Srinivasan, G.||Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation: Proceedings of the ESO Workshop Held at Garching, Germany, 6-8 September 1999, in Honour of Riccardo Giacconi, ESO ASTROPHYSICS SYMPOSIA. Eds. L. Kaper, E.P.J. van den Heuvel, and P.A. Woudt. p45, Springer-Verlag, 2001.
||1981 ||On the morphology of supernova remnants||Radhakrishnan, V.; Srinivasan, G.||Advances in Space Research, 1981, Vol.1, p95-98
||20-May-1984 ||On the nature of the Supernova Remnant 0540-69.3 in the large Magellanic cloud||Srinivasan, G.; Bhattacharya, D.||Current Science, 1984, Vol. 53, p513 -516.
||1985 ||On the nature of the supernova remnant O540-69.3 in the large magellanic cloud||Bhattacharya, D.; Srinivasan, G.||Proceedings of the Academy Workshop on Supernovae, their Progenitors and Remnants, October 29-November 2, 1984, Raman Research Institute, Bangalore. Eds, G. Srinivasan, V. Radhakrishnan; Indian Academy of Sciences, Bangalore, 1985, p119
||5-Dec-1982 ||On the origin of the recently discovered ultra-rapid pulsar||Radhakrishnan, V.; Srinivasan, G.||Current Science, 1982, Vol. 51, p1096-1099.
||27-Feb-1973 ||On the plasmon-theory of the surface energy of metals||Jonson, M.; Srinivasan, G.||Physics Letters, 1973, Vol.43A, p.427