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  • Shylaja, B. S (International Astronomical Union, 1987)
    The binaries with subgroup WN components have been chosen, with periods ranging from 1.64 d to 21.63 d, for understanding the effect of the companion on the formation of this line.
  • Simmons, W. J (Astronomical Society of India, 1915)
  • The Times of India (The Times of India, 2023-09-02)
  • Smith, C. M (Wiley, 1910-03)
  • Park, C; Pranav, P; Pravabati, C; Weygaert, R; Jones, B; Vegter, G; Kim, I; Hidding, J; Hellwing, W. A (The Korean Astronomical Society, 2013-06)
    We present the relation between the genus in cosmology and the Betti numbers for excursion sets of three- and two-dimensional smooth Gaussian random fields, and numerically investigate the Betti numbers as a function of ...
  • Sreekumar, P; Koteswara Rao, V (Indian Academy of Science, 2021-10)
    India has an expanding program in using space as a platform for research. Astrophysics research from satellites increasingly complement ground-based observations with unique wavelength coverage, more frequent temporal ...
  • Birdie, C; Vijaya Lakshmi, B (IATUL (International Association of Scientific and Technological Universities Libraries), 2003)
  • Brilenkov, M; Fornazier, K. S. F; Hergt, L. T; Hoerning, G. A; Marins, A; Murokoshi, T; Fazlu Rahman; Stutzer, N-O; Zhou, Y; Abdalla, F. B; Andersen, K. J; Aurlien, R; Banerji, R; Basyrov, A; Battista, A; Bersanelli, M; Bertocco, S; Bollanos, S; Colombo, L. P. L; Eriksen, H. K; Eskilt, J. R; Foss, M. K; Franceschet, C; Fuskeland, U; Galeotta, S; Galloway, M; Gerakakis, S; Gjerløw, E; Hensley, B; Herman, D; Hoang, T. D; Ieronymaki, M; Ihle, H. T; Jewell, J. B; Karakci, A; Keihänen, E; Keskitalo, R; Maggio, G; Maino, D; Maris, M; Paradiso, S; Partridge, B; Reinecke, M; Suur-Uski, A-S; Svalheim, T. L; Tavagnacco, D; Thommesen, H; Tomasi, M; Watts, D. J; Wehus, I. K; Zacchei, A (EDP Sciences, 2023-07)
    End-to-end simulations play a key role in the analysis of any high-sensitivity cosmic microwave background (CMB) experiment, providing high-fidelity systematic error propagation capabilities that are unmatched by any other ...
  • Kameswara Rao, N; Vagiswari, A; Birdie, C (Indian Academy of Sciences, 2014-02-25)
    In the last decade of the 19th century Maharaja Takhtasingji Observatory was built at Poona (1888–1912) under the supervision of K. D. Naegamvala, with the grant from Maharaja of Bhavnagar (from where the name Bhavnagar ...
  • Senthil Kumar, N; Radhakrishnan, N; Hadimani, Nagesh; Prabahar, P (Journal of Advances in Library and Information Science, 2018-01)
    Bibliometrics is one of the techniques to analyze the quantitative literature and can be applied to research articles published in national, international journals on related articles. This paper deals with the bibliometric ...
  • Iqbalahmad, U. Rajgoli; Ghouse Modin, N. Mamdapur; Prabahar, P (JALIS, 2017-03)
    The bibliometric portrait of Journal of the Indian Society of Remote Sensing concentrates on four decades publication trends from 1973-2014. The study analyzed 1310 research articles published in 140 issues of the journal. ...
  • Anupama, G. C; Subhasis, Chattopadhyay; Deshpande, Shishir; Ghosh, Joydeep; Godbol, Rohini M; Indumathi, D; Souradeep, Tarun (Nature Publishing Group, 2021-11)
    Current and future big science projects in India are providing opportunities for young researchers and building technological capabilities, while contributing to new scientific discoveries. Seven scientists involved in ...
  • Miroshnichenko, A. S; Zharikov, S.V; Korcakova, D; Manset, N; Mennickent, R; Khokhlov, S. A; Danford, S; Raj, A; Zakhozhay, O.V (Astronomical Institute of the Slovak Academy of Sciences, 2020-03)
    Many B-type stars exhibit two phenomena that are symbolized Be and B[e]. The former refers to presence of a circumstellar gaseous disk without significant circumstellar dust, while the latter have dust. Although neither ...
  • Sahai, R; Contreras, C. S; Mangan, A. S; Sanz-Forcada, J; Muthumariappan, C; Claussen, M. J (IOP Publishing, 2018-06-20)
    Binarity is believed to dramatically affect the history and geometry of mass loss in AGB and post-AGB stars, but observational evidence of binarity is sorely lacking. As part of a project to search for hot binary companions ...
  • Bardoloi, I; Baruah, Mon Moyuri (Astronomical Society of India, 2004-03)
    A thermonuclear model for x-ray transients has been considered to explain the observed characteristics of x-ray transient outbursts in Aql X-1, Cen X-4, 1608-522. The model is of a compact primary neutron star (NS) in a ...
  • Konar, S (Astronomical Society of India, 2003)
    There has been strong observational evidence suggesting a casual connection between the binary history of neutron stars and the evolution of their magnetic field. In this article we discuss one of 3 the plausible mechanisms ...
  • Narlikar, J. V (Astronomical Society of India, 1979-03)
  • Sutantyo, W (Astronomical Society of India, 1974-12)
  • Mohanty, D. K (Astronomical Society of India, 1974-12)
  • Sengupta, S (Elsevier, 2000-07)
    A binary stellar system loses its orbital rotational energy by the emission of gravity wave. If there exists a charge asymmetry between electron and proton then the system would also lose its orbital rotational energy due ...

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