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Browsing by Author "Srinivasan, G."

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Issue DateTitleAuthor(s)Citation
1980 Evidence for a large population of shocked interstellar cloudsRadhakrishnan, V.; Srinivasan, G.Journal of Astrophysics and Astronomy, 1980, Vol. 1, p47-66.
1991 The evolution of neutron star magnetic fieldsBhattacharya, D.; Srinivasan, G.Neutron Stars, Proceedings of the NATO Advanced Study Institute, held in Agia Pelagia, Crete, Greece, Sept. 3-14, 1990, Dordrecht: Kluwer, 1991, eds. Joseph Ventura and David Pines. NATO Advanced Science Institutes (ASI) Series C, Vol.344, p219
1991 Evolution of the magnetic fields of neutron starsSrinivasan, G.Texas / Eso-Cern Symposium on Relativistic Astrophysics, Cosmology, and Fundamental Physics Vol647, p.538-547
1991 Evolution of the magnetic fields of neutron starsSrinivasan, G.Annals of the New York Academy of Sciences, 1991, Vol.647, p538-547
1988 Evolution of the morphology of supernova remnants with pulsarsSrinivasan, G.; Bhattacharya, D.Supernova Shells and Their Birth Events. Proceedings of a Workshop held at the Physikzentrum Bad Honnef, March 7-11, 1988. Editor, Wolfgang Kundt; Publisher, Springer-Verlag, Berlin, Germany, New York, NY, 1988.
11-Feb-1991 Gamma rays from millisecond pulsars.Bhattacharya, D.; Srinivasan, G.Journal of Astrophysics and Astronomy, 1991, Vol. 12, p17-25.
Mar-2001 GMRT observations of interstellar clouds in the 21cm line of atomic hydrogen.Mohan, Rekhesh; Dwarakanath, K.S.; Srinivasan, G.; Chengalur, J.N.Journal of Astrophysics and Astronomy, 2001, Vol.22, p35
2002 HI 21 cm-line observations with the GMRT towards interstellar clouds previously seen in optical absorptionMohan, Rekhesh; Dwarakanath, K.S.; Srinivasan, G.; Chengalur, J.N.IAU Symposium, 2002, Vol.199, p341
2004 A high galactic latitude HI 21 cm-line absorption survey using the GMRT: II. Results and interpretationMohan, Rekhesh; Dwarakanath, K.S.; Srinivasan, G.Journal of Astrophysics and Astronomy, 2004, Vol. 25, p185-202.
2004 A high galactic latitude HI 21cm-line absorption survey using the GMRT: I. observations and spectraMohan, Rekhesh; Dwarakanath, K.S.; Srinivasan, G.Journal of Astrophysics and Astronomy, 2004, Vol. 25, p143-183.
1985 How often are remnants like the Crab Nebula bornDwarakanath, K.S.; 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, p97-103
1998 The interstellar clouds of Adams and Blaauw revisited: An HI absorption study - IIRajagopal, Jayadev; Srinivasan, G.; Dwarakanath, K.S.Journal of Astrophysics and Astronomy, 1998, Vol. 19, p117-131.
1998 The interstellar clouds of Adams and Blaauw revisited: An HI absorption study - IRajagopal, Jayadev; Srinivasan, G.; Dwarakanath, K.S.Journal of Astrophysics and Astronomy, 1998, Vol. 19, p97-116.
1995 The interstellar medium surrounding the Vela supernova remnantSaravanan, T.P.; Deshpande, A.A.; Srinivasan, G.Journal of Astrophysics and Astronomy Supplement, 1995, Vol. 16, p275 -276.
1999 The IRAS Vela shell: a "super shell" in the making?Rajagopal, Jayadev; Srinivasan, G.IAU Symposium, 1999, Vol.190, p160
25-Jul-1993 Jan Hendrik OortSrinivasan, G.Current Science, 1993, Vol. 65, p133-134.
Oct-1977 Magnetic field induced Wigner transition in inversion layersJonson, M.; Srinivasan, G.Solid State Communications, 1977, Vol.24, p61-64
1995 The magnetic fields of neutron stars and their evolutionBhattacharya, D.; Srinivasan, G.X-ray binaries Eds. W. H. G. Lewin et al. Cambridge University, 1995, p495-522
2012 Maps of TimeSrinivasan, G.Think, 2012
22-Apr-2002 The maximum mass of neutron starsSrinivasan, G.THE ASTRONOMY AND ASTROPHYSICS REVIEW, 2002, Vol.11, p.67
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