1. IIA Institutional Repository

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Issue DateTitleAuthor(s)
1986Abundance analysis of R CrB variable UW CENGiridhar, S; Kameswara Rao, N
1983-06The chemical composition of Algol systems. II - The carbon and nitrogen abundances of the secondaries of U CEP and U SGEParthasarathy, M; Lambert, D. L; Tomkin, J
1994-12The chemical composition of the RV Tauri variable IW CarinaeGiridhar, S; Kameswara Rao, N; Lambert, D. L
1981-09A compilation of physical parameters of AP and AM stars as derived from energy distribution studiesBabu, G. S. D; Shylaja, B. S
1983-09Density dependence of the line source functions in scattering mediaPeraiah, A
1988Detection of a branching-off feature from the Cygnus-Orion arm in the direction of CarinaBabu, G. S. D
1980Effects of high radial velocities on line transfer in extended atmospheresPeraiah, A
1990-02Effects of rotation on colours and line indices of stars. III - Binary and peculiar starsRajamohan, R; Mathew, A
1994-10Embedded clusters in giant extragalactic H II regions, 1: BVRH-alpha photometryMayya, Y. D
1990-09Expanding shell and P Cygni profiles of 27 Canis MajorisGhosh, K. K
1989-05Flare-like activity in Be stars HR 7403 and .8762Ghosh, K. K
1984-08Frequency shifts and line broadening of radiation from rotating neutron starsKapoor, R. C; Datta, B
1988Further spectroscopic observations of SN 1987AAnupama, G. C; Prabhu, T. P; Ghosh, K. K; Ashoka, B. N; Giridhar, S
1982-05HD 81410 - A new RS CVn binaryRaveendran, A. V; Mekkaden, M. V; Mohin, S
1983Identification of new CeO features in the S star Pi GruisMurty, P. S
1977-02K emission line widths in the sun and the starsBappu, M. K. V; Sivaraman, K. R
1982-03K2V/K2R asymmetries in the sun and starsSivaraman, K. R
1978-09Line formation in spherical media with partial frequency redistribution. I - Solution of the line transferPeraiah, A
1979-07Line formation in spherical media with partial frequency redistribution. II - Expanding media with redistribution function R sub IPeraiah, A
1982New identifications of YO and CeO in R CygniMurty, P. S
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