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Issue DateTitleAuthor(s)Citation
Jun-2007 Can you see air?Narayanan, Andal; Samuel, J.; Sinha, SupurnaResonance, 2007, Vol.12 (June), p71-75
Caravan of Indian nation will pass on: Sir C.V.Raman's criticism of universities - a scientific remedy--
Nov-2011 Carbon-based liquid crystals: art and scienceBisoyi, Hari Krishna; Kumar, SandeepLiquid Crystals, 2011, Vol.38, p1427-1449
1929 Carbon compounds: their magnetic behaviour - Prof. Raman's researches-The Hindu, 1929
28-Jul-2010 Carbon ionization states and the cosmic far-UV background with He II absorptionVasiliev, Evgenii O.; Sethi, S.K.; Nath, Biman B.Astrophysical Journal, 2010, Vol. 719, p1343
14-Feb-2003 Carbon Nanotube Flow SensorsGhosh, Shankar; Sood, A.K.; Kumar, N.Science, 2003, Vol.299, p1042-1044
2009 Carbon nanotubes in discotic liquid crystalsBisoyi, Hari Krishna; Kumar, SandeepJournal of Indian Institute of Science, 2009, Vol. 89, p101-112
May-2008 Carbon nanotubes in triphenylene and rufigallol-based room temperature monomeric and polymeric discotic liquid crystalsBisoyi, Hari Krishna; Kumar, SandeepJournal of Materials Chemistry, 2008, Vol.18, p3032
23-May-2003 Carbon Nanotubes Provide a ChargeCohen, Adam E.; Ghosh, Shankar; Sood, A.K.; Kumar, N.Science, 2003, Vol.300, p1235 - 1236
2002 Carbon recombination lines at 34.5 MHz from the galactic planeKantharia, N.G.; Anantharamaiah, K.R.IAU Symposium, 2002, Vol.199, p347
20-Oct-1998 Carbon recombination lines between 34.5 and 770 MHz. toward Cassiopeia AKantharia, N.G.; Anantharamaiah, K.R.; Payne, H.E.The Astrophysical Journal, 1998, Vol.506, p.758-772
2001 Carbon recombination lines from the galactic plane at 34.5 & 328 MHzKantharia, N.G.; Anantharamaiah, K.R.Journal of Astrophysics and Astronomy, 2001, Vol.22, p51-80.
Sep-2002 Carbon recombination lines near 327 MHz. I. ``Diffuse'' C II regions in the Galactic DiskRoshi, Anish D.; Kantharia, N.G.; Anantharamaiah, K.R.Astronomy and Astrophysics, 2002, Vol.391, p1097-1113
Jun-2011 Carbon recombination lines towards the Riegel-Crutcher cloud and other cold HI regions in the inner galaxyRoshi, Anish D.; Kantharia, N.G.Monthly Notices of the Royal Astronomical Society, 2011, Vol.414, p519
10-Mar-1949 Care of the human eye : Sir C .V. Raman's appeal , Opthalmologists conference in the city-The Hindu, 1949
1993 A case for no decay of the magnetic fields of isolated radio pulsarsWijers, R.A.M.J.; Verbunt, F.; Bhattacharya, D.; Hartman, J.M.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
1996 The case for no field decay from improved pulsar population studiesHartman, J.W.; Verbunt, F.; Bhattacharya, D.; Wijers, H.IAU Colloquium, 1996, Vol.160, p47
20-Jan-2002 A case for renewed activity in the giant radio galaxy J0116-473Saripalli, Lakshmi; Subrahmanyan, Ravi; Udaya Shankar, N.Astrophysical Journal, 2002, Vol.565, p256-264
Nov-1999 Causal continuity in degenerate spacetimesBorde, A.; Dowker, H.F.; Garcia, R.S.; Sorkin, Rafael D.; Surya, SumatiClassical and Quantum Gravity, 1999, Vol.16, Issue 11, p 3457-3481
Oct-1981 Causality conditions and the lengths of nonspacelike curvesDhurandhar, S.V.; Joshi, P.S.General Relativity and Gravitation, 1981, Vol.13, p913
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