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  • 1-D dusty photo-ionization models of WR planetary nebulae NGC 2452 and IC 2003 
    Muthumariappan, C; Amrutha, B. M; Selvakumar, G (Elsevier B.V., 2023-01-01)
    We report dusty photo-ionization models for two Planetary Nebulae NGC 2452 and IC 2003, which have [WR] type central stars, using 1D photo-ionization code Cloudy17.02. We used the medium resolution optical spectra and ...
  • The 1.28 GHz MeerKAT Galactic Center Mosaic 
    Heywood, I; Rammala, I; Camilo, F; Cotton, W. D; Yusef-Zadeh, F; Abbott, T. D; Adam, R. M; Adams, G; Aldera, M. A; Asad, K. M. B; Bauermeister, E. F; Bennett, T. G. H; Bester, H. L; Bode, W. A; Botha, D. H; Botha, A. G; Brederode, L. R. S; Buchner, S; Burger, J. P; Cheetham, T; de Villiers, D. I. L; Dikgale-Mahlakoana, M. A; du Toit, L. J; Esterhuyse, S. W. P; Fanaroff, B. L; February, S; Fourie, D. J; Frank, B. S; Gamatham, R. R. G; Geyer, M; Goedhart, S; Gouws, M; Gumede, S. C; Hlakola, M. J; Hokwana, A; Hoosen, S. W; Horrell, J. M. G; Hugo, B; Isaacson, A. I; Jozsa, G. I. G; Jonas, J. L; Joubert, A. F; Julie, R. P. M; Kapp, F. B; Kenyon, J. S; Kotze, P. P. A; Kriek, N; Kriel, H; Krishnan, V. K; Lehmensiek, R; Liebenberg, D; Lord, R. T; Lunsky, B. M; Madisa, K; Magnus, L. G; Mahgoub, O; Makhaba, A; Makhathini, S; Malan, J. A; Manley, J. R; Marais, S. J; Martens, A; Mauch, T; Merry, B. C; Millenaar, R. P; Mnyandu, N; Mokone, O. J; Monama, T. E; Mphego, M. C; New, W. S; Ngcebetsha, B; Ngoasheng, K. J; Ockards, M. T; Oozeer, N; Otto, A. J; Passmoor, S. S; Patel, A. A; Peens-Hough, A; Perkins, S. J; Ramaila, A. J. T; Ramanujam, N. M. R; & 30 Co-authors (American Astronomical Society, 2022-02-01)
    The inner ∼200 pc region of the Galaxy contains a 4 million M⊙ supermassive black hole (SMBH), significant quantities of molecular gas, and star formation and cosmic-ray energy densities that are roughly two orders of ...
  • `1.3-Year' and `153-day' Periodicities in the Sun's Surface Rotation 
    Javaraiah, J (Astronomical Society of India, 2003)
    Using the daily Mt. Wilson velocity data during 1986-1994, we found 1.3 ± 0.1 yr periodicity - is dominant in the Sun's surface `mean' rotation rate (A ) during 1986-1994 (solar cycle 22). A 153 ± 5 - day periodicity found ...
  • 1.5M Aluminizing Plant of the Indian Institute of Astrophysics 
    Saxena, A. K; Jayarajan, A. P; Kumar, K (Indian Institute of Astrophysics, Bangalore, 1980)
    The design and features of 1.5m vacuum coating plant an in house facility at the Kavalur Observatory for periodic aluminizing of astronomical optics are described. A typical performance data is given.
  • 1.8 MeV emission lines from galactic plane region 
    Bardoloi, I; Duorah, K; Duorah, H. L; Barua, M. M (Astronomical Society of India, 1996)
    The COMPTEL telescope aboard the CGRO satellite has revealed highly significant 1.8 MeV emission lines from the Galactic plane region of the Milky Way Galaxy. The observed concentrated emission region may contain a single ...
  • 10 scientists get UGC's Hari Om Trust awards 
    The Hindu (The Hindu, 1981-10-01)
  • A 10-m class national large optical-IR telescope 
    Anupama, G. C; Maheswar, G; Sriram, S; Sivarani, T; Parihar, P. S; Nagabhushana, S; Angchuk, D; Barway, Sudhanshu; Bhatt, B. C; Banyal, R. K; Basheer, Alikhan; Prasanna, Deshmukh; Divakar, D. K; Dorjai, T; Goswami, A; Govinda, K. V; Jorphail, S; Kamath, U. S; Kemkar, P. M. M; Mahay, T. T; Muneer, S; Muthumariappan, C; Shantikumar, N. S; Pandey, G; Reddy, B. E; Sahu, D. K; Sandeep, D. S; Ramya, S; Stalin, C. S; Subramanian, S; Tsewang, Stanzin; Subramaniam, A (Indian Academy of Science, 2022-06)
    An observatory class national large optical-IR telescope (NLOT), is proposed to be built and located in the country. The telescope consists of a 10–12 m segmented primary. In order to cater to a diversity of observational ...
  • 100 years of photon-counting: the quest for the perfect eye 
    Morel, S; Saha, S. K (Anita Publications, 2005)
  • The 1024 channel digital correlator receiver of the Gauribidanur radioheliograph 
    Ramesh, R; Sundararajan, M. S; Sastry, Ch. V (Springer, 2006-02)
    A low frequency (40 150 MHz) radioheliograph for observations of the solar corona is in operation for the last few years at the Gauribidanur radio observatory, about 100 km north of Bangalore. The array has 32 antenna ...
  • The 14th International Conference on Cosmic Rays 
    Daniel, R. R (Astronomical Society of India, 1975-09)
  • The 16th International Cosmic Ray Conference 
    Daniel, R. R (Astronomical Society of India, 1979-12)
  • 1840 - 1880 Chintamanny Ragoonatha Chary 
    Indian Institute of Astrophysics (Indian Institute of Astrophysics, 2006)
  • 1947 - A love story (with maths!) 
    Deccan Herald (Deccan Herald, 1999-08-03)
  • The 1985 outburst of RS Ophiuchi - Spectroscopic results 
    Anupama, G. C; Prabhu, T. P (Indian Academy of Sciences, 1989-09)
    Results are reported from visual spectroscopy of the recurrent nova RS Oph, obtained with a Cassegrain spectrograph on the 102-cm reflector at Vainu Bappu Observatory in February-May 1985 (days 32-108 postoutburst). The ...
  • 1986 Light Curve of V711 Tau 
    Mekkaden, M. V (Konkoly Observatory, 1987-07-03)
  • The 1995 Total Solar Eclipse: An Overview 
    Singh, J (Indian Institute of Astrophysics, 1997)
    As we know, we owe the discovery of solar corona to the observation of total solar eclipse. Inspite of all that has been learned, coronal studies still remain the most important aspect of scientific investigation during ...
  • The 1995-96 decline of R Coronae Borealis: high-resolution optical spectroscopy 
    Kameswara Rao, N; Lambert, D. L; Adams, M. T; Doss, D. R; Gonzalez, G; Hatzes, A. P; James, C. R; Johns-Krull, C. M; Luck, R. E; Pandey, G; Reinsch, K; Tomkin, J; Woolf, V. M (The Royal Astronomical Society, 1999-12)
    A set of high-resolution optical spectra of R CrB acquired before, during and after its 1995-96 decline is discussed. All of the components reported from earlier declines are seen. This novel data set provides new information ...
  • 1998 activity of Leonid meteor shower 
    Lokanadham, B; Yellaiah, G; Kalyan Kumar, J; Bheemeshwer Rao, S; Chandrasekhar Rao, V (Astronomical Society of India, 2000)
    A group of five observers have participated in visual, photographic and MST radar observations of Leonid meteor shower during 15-20 November 1998 at National MST Radar Facility (NMRF), Gadanki (13.47 deg N, 79.18 deg E) ...
  • The 1999 Outburst of the Recurrent Nova U Scorpii 
    Anupama, G. C; Dewangan, G. C (The American Astronomical Society, 2000-03)
    The optical spectra of the recurrent nova U Sco obtained in five epochs 0.45-42.35 days after the 1999 outburst maximum are presented here. For the first time, an outburst spectrum of U Sco has been obtained as early as ...
  • 1D radiative transfer models of 21 and 30 μm emission features in proto-planetary nebulae 
    Muthumariappan, C; Reddy, B. E (Cambridge University Press, 2012-08)
    Spectral energy distributions of six proto-planetary nebulae showing 21 and 30μ features were fit with models obtained from 1D radiative transfer code, taking FeO and MgS respectively are the carriers of the features. ...

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