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Browsing IIAP Publications by Title

Browsing IIAP Publications by Title

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  • Jain, S. K; Bhatt, H. C; Sagar, R (The American Physical Society, 1990-05)
    The linear polarization of eight bright Herbig Ae/Be stars in UBVRI bands has been measured. No unique wavelength dependence of polarization magnitude or direction is found in these measurements. Comparison with earlier ...
  • Banyal, R. K; Prasad, B. R (Indian Academy of Sciences, 2007-03)
    We report the pump--probe measurements of nonlinear refractive index changes in photochromic bacteriorhodopsin films. The photoinduced absorption is caused by pump beam at 532 nm and the accompanying refractive ...
  • Jha, Bibhuti K; Priyadarshi, Aditya; Mandal, Sudip; Chatterjee, Subhamoy; Banerjee, D (Springer, 2021-01)
    The rotational profile of the Sun is considered to be one of the key inputs in a solar dynamo model. Hence, precise and long-term measurements of this quantity is important for our understanding of solar magnetism and its ...
  • Singh, V; Shastri, P; Risaliti, G (EDP Sciences, 2011-09)
    Context. The unification scheme of Seyfert galaxies hypothesizes that Seyfert type 1s and type 2s are intrinsically similar and the observed differences between the two subtypes are solely due to the differing orientations ...
  • de Sabbata, V; Sivaram, C (International Cosmic Ray, 1990)
  • Knowles, K; Cotton, W. D; Rudnick, L; Camilo, F; Goedhart, S; Deane, R; Ramatsoku, M; Bietenholz, M. F; Bruggen, M; Button, C; Chen, H; Ranchod, S; Retana-Montenegro, E; Sebokolodi, L; Sikhosana, S. P; Smirnov, O; Cheetham, T; Thorat, K; Venturi, T; Abbott, T. D; Adam, R. M; Kotze, A. G; Adams, G; Aldera, M. A; Bauermeister, E. F; Bennett, T. G. H; Bode, W. A; Botha, D. H; de Villiers, D. I. L; Botha, A. G; Dikgale-Mahlakoana, M. A; du Toit, L. J; Kriek, N; Esterhuyse, S. W. P; Fadana, G; Fanaroff, B. L; Manley, J. R; Fataar, S; Foley, A. R; Fourie, D. J; Frank, B. S; Gamatham, R. R. G; Gatsi, T. G; Kriel, H; Geyer, M; Gouws, M; Gumede, S. C; Heywood, I; Marais, S. J; Hlakola, M. J; Hokwana, A; Hoosen, S. W; Horn, D. M; Horrell, J. M. G; Krishnan, V. K; Hugo, B. V; Isaacson, A. R; Jonas, J. L; Jordaan, J. D. B; Joubert, A. F; Maree, M. D. J; Julie, R. P. M; Kapp, F. B; Kasper, V. A; Kenyon, J. S; Kusel, T. W; Kotze, P. P. A; Martens, A; Legodi, L. S; Lehmensiek, R; Liebenberg, D; Lord, R. T; Taljaard, B; Lunsky, B. M; Madisa, K; Magnus, L. G; Main, J. P. L; Makhaba, A; Makhathini, S; Mauch, T; Malan, J. A; McAlpine, K; Merry, B. C; Tasse, C; Millenaar, R. P; Mokone, O. J; Monama, T. E; Chibueze, J. O; Mphego, M. C; New, W. S; Ngcebetsha, B; Ngoasheng, K. J; Ockards, M. T; Otto, A. J; Tiplady, A. J; Patel, A. A; Peens-Hough, A; Perkins, S. J; Ramanujam, N. M; Clarke, T. E; Ramudzuli, Z. R; Ratcliffe, S. M; Renil, R; Robyntjies, A; Rust, A. N; Toruvanda, O; Salie, S; Sambu, N; Schollar, C. T. G; Schwardt, L. C; Schwartz, R. L; Gasperin, F. de; Serylak, M; Siebrits, R; Sirothia, S. K; Slabber, M; Twum, S. N; Sofeya, L; Ianjamasimanana, R; van Balla, T. J; van der Byl, A; van der Merw, C; van Dy, C. L; Brederode, L. R. S; Van Tonder, V; Van Wyk, R; Venter, A. J; Venter, M; Welz, M. G; William, L. P; Jozsa, G. I. G; Xaia, B; Hilton, M; Kesebonye, K. C; Buchner, S; Kolokythas, K; Kraan-Korteweg, R. C; Lawrie, G; Lochner, M; Loubser, S. I; Marchegiani, P; Mhlahlo, N; Moodley, K; Murphy, E; Namumba, B; Burger, J. P; Oozeer, N; Parekh, V; Pillay, D. S; Passmoo, S. S; Ramaila, A. J. T (EDP Sciences, 2022-01)
    MeerKAT’s large number (64) of 13.5 m diameter antennas, spanning 8 km with a densely packed 1 km core, create a powerful instrument for wide-area surveys, with high sensitivity over a wide range of angular scales. The ...
  • Babu, G. S. D (Indian Academy of Sciences, 1983-12)
    Low-dispersion spectra of the order of 1000 Å mm-1 have been obtained for stars in several faint galactic clusters with a transmission grating placed in front of the photographic plate at the Cassegrain focus of the Kavalur ...
  • Bayanna, A. R; Louis, R. E; Chatterjee, S; Mathew, S. K; Venkatakrishnan, P (Optical Society of America, 2015-03-01)
    A deformable mirror (DM) is an important component of an adaptive optics system. It is known that an on-axis spherical/parabolic optical component, placed at an angle to the incident beam introduces defocus as well as ...
  • Bhargava, B. N; Saha, A. K (Kodaikanal Observatory, Kodaikanal, 1967)
  • Srinivasa Prasannaa, V; Vutha, A. C; Abe, M; Das, B. P (The American Physical Society, 2015-05)
    Heavy polar diatomic molecules are the primary tools for searching for the T-violating permanent electric dipole moment of the electron (eEDM). Valence electrons in some molecules experience extremely large effective ...
  • Sivaram, C (International Union of Pure and Applied Physics, 1995)
    Two possible merger modes of gamma ray bursts are considered. The merger of two white dwarfs leading to a neutrino bursts accompanying the gamma ray burst. However the merger of two neutron stars should give rise to only ...
  • Rajaguru, S. P; Antia, H. M (IOP Publishing, 2015-11-10)
    We present and discuss results from time–distance helioseismic measurements of meridional circulation (MC) in the solar convection zone using 4 yr of Doppler velocity observations by the Helioseismic and Magnetic Imager ...
  • Sbordone, L; Bonifacio, P; Caffau, E; Ludwig, H. -G; Behara, N. T; González Hernández, J. I; Steffen, M; Cayrel, R; Freytag, B; Van’t Veer, C; Molaro, P; Plez, B; Sivarani, T; Spite, M; Spite, F; Beers, T. C; Christlieb, N; François, P; Hill, V (EDP Sciences, 2010-11)
    Context. The primordial nature of the Spite plateau is at odds with the WMAP satellite measurements, implying a primordial Li production at least three times higher than observed. It has also been suggested that A(Li) might ...
  • Pinto, A. M. Matas; Spite, M; Caffau, E; Bonifacio, P; Sbordone, L; Sivarani, T; Steffen, M; François, P; Di Matteo, P (EDP Sciences, 2021-10)
    Context. The study of old, metal-poor stars deepens our knowledge on the early stages of the universe. In particular, the study of these stars gives us a valuable insight into the masses of the first massive stars and their ...
  • Gurumath, S. R; Hiremath, K. M; Ramasubramanian, V (Indian Academy of Sciences, 2017-07)
    By considering the physical and orbital characteristics of G type stars and their exoplanets, we examine the association between stellar mass and its metallicity that follows a power law. Similar relationship is also ...
  • Sbordone, L; Bonifacio, P; Caffau, E; Ludwig, H. -G; Behara, N; Gonzalez-Hernandez, J. I; Steffen, M; Cayrel, R; Freytag, B; Van't Veer, C; Molaro, P; Plez, B; Sivarani, T; Spite, M; Spite, F; Beers, T. C; Christlieb, N; François, P; Hill, V (Cambridge University Press, 2010-03)
    We present the largest sample available to date of lithium abundances in extremely metal poor (EMP) Halo dwarfs. Four Teff estimators are used, including IRFM and Hα wings fitting against 3D hydrodynamical synthetic ...
  • Sbordone, L; Bonifacio, P; Caffau, E; Ludwig, H. -G; Behara, N; Gonzalez-Hernandez, J. I; Steffen, M; Cayrel, R; Freytag, B; Van't Veer, C; Molaro, P; Plez, B; Sivarani, T; Spite, M; Spite, F; Beers, T. C; Christlieb, N; François, P; Hill, V (Cambridge University Press, 2010-04)
    We recently presented (Sbordone et al., 2009a) the largest sample to date of lithium abundances in extremely metal-poor (EMP) Halo dwarf and Turn-Off (TO) stars. One of the most crucial aspects in estimating Li abundances ...
  • Das, Tanya; Banyal, R. K (Optical Society of America, 2021-11-01)
    Technological advancement has led to improvement in the design capabilities of astronomical spectrographs, allowing for high-precision spectroscopy, thereby expanding the realms of observational astronomy. High-resolution ...
  • Maheswar, G; Lee, C. W; Bhatt, H. C; Mallik, S. G. V; Dib, S (EDP Sciences, 2010-01)
    We aim to develop a method to determine distances to molecular clouds using JHK near-infrared photometry. Methods: The method is based on a technique that aids spectral classification of stars lying towards the fields ...
  • Ramesh, R; Kathiravan, C; Satya Narayanan, A; Ebenezer, E (The European Southern Observatory, 2003-03)
    We present metric radio observations of quasi-periodic emission from the solar corona in close association with a ``halo'' CME and an ``EIT wave'' phenomenon. The radio event lasted for about 60 s. Its mean periodicity was ...

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