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Issue DateTitleAuthor(s)
1986-03Boundary to the solar system set by the Galaxy according to King-Innanen's formulaRawal, J. J
2000CCD photometry of the Wolf Rayet galaxy MinkSingh, M; Sanwal, B. B; Stalin, C. S
2000Chemical evolution of intermediate mass nuclei in the solar neighbourhood and the halo of the galaxyGoswami, A; Prantzos, N
2012Classical Be stars in our Galaxy and the Magellanic CloudsSubramaniam, A; Mathew, B; Paul, K. T; Mennickent, R. E; Sabogal, B
2005-12A deep focus on NGC 1883Tadross, A. L
2009-06Design and analysis of an FUV spectrograph for a small satelliteMunshi, R; Prasad, B. R; Murthy, J
1998Distribution of Dark Matter in the GalaxyRatnam, Charu
1997-01Galactic Age Estimates from O-rich Stardust in MeteoritesNittler, L. R; Cowsik, R
1995-06Galaxy dynamics with small computers: Some results on tidal interactions.Kochhar, R. K; Namboodiri, P. M. S
2003GMRT Neutral Hydrogen Observations of the Sombrero GalaxySengupta, C; Balasubramanyam, R; Bekki, K
1993A gravitational lens probe of galaxy-scale dark matter?Sunita Nair
1993-07-25Jan oort and interstellar cloudsMallik, D. C. V
2001-03The Luminosity Function and Size Distribution of HII Regions in NGC 1365Ravindranath, S; Prabhu, T. P
2013-06Mapping extinction using GALEX and SDSS photometric observationsPreethi, K; Gudennavar, S. B; Murthy, J
2002The Mass Function of Young Star Clusters in our Galaxy and Nearby Galaxies: Is It Universal?Sagar, R
1993A maximum entropy method based scheme for the inversion of extended radio images in gravitationally lensed systemsSunita Nair
2012-10Multiwavelength Study of the NGC 281 RegionSharma, S; Pandey, A. K; Pandey, J. C; Chauhan, N; Ogura, K; Ojha, D. K; Borrissova, J; Mito, H; Verdugo, T; Bhatt, B. C
2003Near Infrared Survey of the Galactic Nuclear Bulge RegionBaliyan, K. S; Ganesh, S; Joshi, U. C; Glass, I. S
1998Observational studies of planetary nebulae with moderate-size telescopesMallik, D. C. V
1995-10Probable binary open star clusters in the Galaxy.Subramaniam, A; Gorti, U; Sagar, R; Bhatt, H. C
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