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| Issue Date | Title | Author(s) | Citation |
|---|---|---|---|
| 1990 | Thermal field growth in neutron stars - An alternative to injection | Bhattacharya, D. | Proceedings of the NATO Advanced Study Institute on Neutron Stars: Their Birth, Evolution, Radiation and Winds, held in Erice, Sicily, Italy, September 5-17, 1988. Neutron stars and their birth events. Ed. Wolfgang Kundt; Publisher, Kluwer Academic Publishers, Dordrecht, The Netherlands; Boston, 1990, p133 |
| 1990 | Millisecond pulsars - A new population of gamma Ray sources | Srinivasan, G. | Proceedings of the NATO Advanced Study Institute on Neutron Stars: Their Birth, Evolution, Radiation and Winds, held in Erice, Sicily, Italy, September 5-17, 1988. Neutron stars and their birth events. Ed. Wolfgang Kundt; Publisher, Kluwer Academic Publishers, Dordrecht, The Netherlands; Boston, 1990, p107 |
| 1978 | A new approach to making large telescope mirrors | Ramaseshan, S.; Rajagopalan, S.R.; Nityananda, R.; Radhakrishnan, V. | Proceedings of the ESO Conference on Optical Telescopes of the Future, Geneva, 1977. Eds. F. Pacini et al. ESO, p371-372 |
| 1985 | A search for compact sources in supernova remnants | Van Gorkom, J.H.; Ekers, R.D.; Johnston, K.; Radhakrishnan, V.; Salter, C.J. | 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, p93 |
| 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 |
| 1985 | On the meaning of pulsar velocities | Radhakrishnan, V.; Shukre, C.S. | 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, p155 |
| 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 |
| 1993 | A case for no decay of the magnetic fields of isolated radio pulsars | Wijers, R.A.M.J.; Verbunt, F.; Bhattacharya, D.; Hartman, J.W. | Isolated Pulsars, Proceedings of the Los Alamos workshop, held in Taos, New Mexico, February 23-28, 1992. Eds. K.A. Riper, R. Epstein and C. Ho. Cambridge: Cambridge University Press, 1993., p.83 |
| 24-Feb-1988 | Specke interferometry of SN 1987A and the "Mystery spot" | Nityananda, R. | Kodaikanal Observatory Bulletin, 1988, Vol.10, p55-58 |
| 1989 | The Decameterwave radio telescope at Gauribidanur: Antenna arrays and control system | Deshpande, A.A.; Shevgaonkar, R.K.; Sastry, Ch.V. | journal of the Institution of Electronics and Telecommunications Engineering, 1989, Vol.35, p342-347 |
| 1988 | Why the Barker sequence bit length does not exceed thirteen? | Rao, B.V.; Deshpande, A.A. | Journal of the Institution of Electronics and Telecommunications Engineering, 1988, Vol.34, p461 |
| 2000 | Pulse fluctuation properties at 35 MHz | Asgekar, Ashish; Deshpande, A.A. | ASP Conference Series, 2000, Vol.202, p161 |
| 1996 | Butcher-Oemler effect and radio continuum | Dwarakanath, K.S.; Owen, F.N. | Cold Gas at High Redshift, Proceedings of a workshop celebrating the 25th anniversary of the Westerbork Synthesis Radio Telescope, held in Hoogeven, The Netherlands, August 28-30, 1995, Dordrecht: Kluwer Academic Publishers, c1996, eds. M.N. Bremer and N. Malcolm. Astrophysics and Space Science Library, Vol. 206, p183-194 |
| 1985 | Gravitational lenses - The multiple scattering limit | Narayan, R.; Nityananda, R. | Extragalactic Energetic Sources, Proceedings of the Winter School on Extragalactic Energetic Sources, Bangalore, January 10-21, 1983. Ed. V. Kapahi. Bangalore: Indian Academy of Sciences, 1985, p149-154 |
| 1990 | Speckle phenomena in inter-planetary scintillation | Cornwell, T.J.; Anantharamaiah, K.R.; Narayan, R. | URSI/IAU Symposium on Radio Astronomical Seeing, Beijing, People's Republic of China, May 15-19, 1989, Proceedings. Beijing/Oxford, International Academic Publishers/Pergamon Press, 1990, p239-242 |
| 1985 | How often are remnants like the Crab Nebula born | Dwarakanath, 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 |
| Jun-1995 | Bright rimmed molecular clouds near massive stars | Indrani, C.; Sridharan, T.K. | Journal of the Astrophysics and Astronomy, 1995, Vol.16, Supplement, p277 |
| 1984 | Are many pulsars processed in binaries | Radhakrishnan, V.; Srinivasan, G. | Proceedings of the Second Asian-Pacific Regional Meeting on Astronomy, held in Bandung, Indonesia, August 24-29, 1981. Editors, B. Hidayat, M.W. Feast; Publisher Tira Pustaka Publishing House, Jakarta, Indonesia, 1984, p423 |
| May-1997 | New results from H92 alpha recombination line observations of NGC 253 | Anantharamaiah, K.R.; Goss, W.M. | Revista Mexicana de Astronomia y Astrofisica Serie de Conferencias, 1997, Vol.6, p58 |
| 1984 | The origin of pulsar velocities | Radhakrishnan, V. | Birth and Evolution of Neutron Stars: Issues Raised by Millisecond Pulsars. Proceedings of the NRAO Workshop, held at the National Radio Astronomy Observatory (NRAO) Green Bank, West Virginia, June 6-8, 1984. Edited by S.P. Reynolds and D.R. Stinebring. Green Bank: National Radio Astronomy Observatory, 1984., p.130 |
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- 70 Pulsars
- 30 galaxies
- 25 Neutron stars
- 24 intergalactic medium
- 23 Galaxies
- 23 reionization
- 23 stars: neutron
- 21 accretion
- 20 radio continuum
- 19 dark ages
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