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Issue DateTitleAuthor(s)Citation
2007 HI content of galaxies in groups.Sengupta, ChandreyeePh.D. Thesis, Jawaharlal Nehru University, New Delhi, 2007.
2005 The HI content of the Eridanus group of galaxiesOmar, A.; Dwarakanath, K.S.Journal of Astrophysics and Astronomy, 2005, Vol. 26, p.71-88.
Oct-2002 Hidden symmetries in deformed microwave resonatorsSamuel, J.; Dhar, AbhishekPhysical Review A, 2002, Vol.66, 044102
Sep-2004 H I deficiency in groups: what can we learn from Eridanus?Omar, A.Bulletin of the Astronomical Society of India, 2004, Vol.32, p239-245
2008 HI Deficiency in X-ray bright groupsBalasubramanyam, R.; Sengupta, Chandreyee; Dwarakanath, K.S.Galaxies in the Local Volume,Astrophysics and Space Science Proceedings, Volume
20-Jul-2006 H I density distribution driven by supernovae: A simulation studyHodge, Jacqueline A.; Deshpande, A.A.Astrophysical Journal, 2006, Vol.646, p232-239
Jul-2007 HI Density Distribution Driven by Supernovae:A Simulation StudyHodge, Jacqueline A.; Deshpande, A.A.ASP Conference Series, Vol. 365, 2007, p158-161
Dec-2003 Hi density distribution driven by supernova ejecta: a simulation studyHodge, Jacqueline A.; Deshpande, A.A.Bulletin of the American Astronomical Society, 2003, Vol.35, p1381
Nov-1992 H I emission and absorption spectra towards the double radio source 1830-211Subrahmanyan, Ravi; Kesteven, Michael J.; te Lintel Hekkert, PeterMonthly Notices of the Royal Astronomical Society, 1992, Vol.259, p63
2009 Hierarchial discsKumar, SandeepLiquid Crystals Today, 2009, Vol.18, p2
2001 HI fluctuations at large redshifts: I–visibility correlationBharadwaj, Somnath; Sethi, S.K.Journal of Astrophysics and Astronomy, 2001, Vol. 22, p293-307
1989 High angular resolution optical interferometryUdaya Shankar, N.Science Focus, 1989, Vol.1, No.2, p8
1989 High angular resolution optical interferometryUdaya Shankar, N.Science Focus, 1989, Vol.1, p8-18
10-Jun-1997 High-Density, Compact H II Regions in the Starburst Galaxies NGC 3628 and IC 694: High-Resolution VLA Observations of the H92 alpha Radio Recombination LineZhao, Jun-Hui; Anantharamaiah, K.R.; Goss, W.M.; Viallefond, F.Astrophysical Journal 1997, Vol.482, p.186-202
Jun-2007 Higher harmonics increase LISA's mass reach for supermassive black holesArun, K.G.; Iyer, B.R.; Sathyaprakash, B.S.; Sinha, SiddharthaPhysical Review D, 2007, Vol.75, p124002
Jul-2009 Higher order nonlinearities in a non-Doppler free geometryNarayanan, Andal; Sharma, A.; Preethi, T.M.; Abheera, H.; Ramachandran, HemaCanadian Journal of Physics, 2009, Vol.87, p 843-850
Nov-2007 Higher signal harmonics, LISA's angular resolution, and dark energyArun, K.G.; Iyer, B.R.; Sathyaprakash, B.S.; Sinha, Siddhartha; Van den Broeck, ChrisPhysical Review D, 2007, Vol.76, p104016-1
Nov-2007 Higher signal harmonics, LISA's angular resolution, and dark energyArun, K.G.; Sathyaprakash, B.S.; Sinha, Siddhartha; Van den Broeck, ChrisPhysical Review D, 2007,Vol.76, 104016
2007 High-frequency carbon recombination line as a probe to study the environment of Ultra-compact HII regionsRoshi, Anish D.Triggered Star Formation in a Turbulent ISM, Edited by B. G. Elmegreen and J. Palous. Proceedings of the International Astronomical Union 2, IAU Symposium #237, held 14-18 August, 2006 in Prague, Czech Republic. Cambridge: Cambridge University Press, 2007., pp.469
1996 A high-frequency radio continuum investigation of giant radio galaxies. II. Observations of four objects at 2.8cm wavelength.Saripalli, Lakshmi; Mack, K.H.; Klein, U.; Strom, R.; Singal, A.K.Astronomy and Astrophysics, 1996, Vol.306, p708
Showing results 1758 to 1777 of 5302
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