Publications of Astronomical Society of India: Recent submissions

  • Mitra, A (Astronomical Society of India, 2002)
    There are many observational evidences for the existence of massive compact condensations in the range 106 - 1010 M? at the core of various galaxies and in particular in the core of High Energy Gamma Ray emitting galaxies. ...
  • Le Coultre, P (Astronomical Society of India, 2002)
    The L3+C experiment takes advantage of the high precision muon spectrometer of the L3 detector installed at LEP, CERN, Geneva, to measure precisely cosmic ray muons. Several physics topics in the field of astrophysics and ...
  • Tonwar, S. C (Astronomical Society of India, 2002)
    Following the discovery of ultra high energy cosmic rays with energies of PeV and higher in the 1950's and detailed studies on the energy spectrum in the TeV-PeV-EeV regions in 1960's, there has been enormous interest in ...
  • Bhat, P. N (Astronomical Society of India, 2002)
    Atmospheric Cverenkov techniques is the only method which has been successfully used to probe the sky in the TeV energy band. However it has certain intrinsic drawbacks arising primarily out of the presence of cosmic rays ...
  • Chakrabarti, S. K (Astronomical Society of India, 2002)
    For the past fifty years, accretion process is being studied initially on normal stars and later, on compact object, such as black holes and neutron stars. In this Review, I present the modern development of this subject ...
  • Böttcher, M (Astronomical Society of India, 2002)
    The current status of leptonic jet models for blazars is reviewed. Differences between the quasar and BL-Lac subclasses of blazars may be understood in terms of the dominance of difference radiation mechanisms in the ...
  • Cowsik, R; Srinivasan, R; Prabhu, T. P (Astronomical Society of India, 2002)
    Situated in the high-altitude cold desert of Changthang Ladakh bordering Himachal Pradesh and Tibet, Indian Astronomical Observatory, Hanle (32o46m46sN, 78o57'51''E; 4500 m above msl), provides excellent opportunities for ...
  • Vishwanath, P. R (Astronomical Society of India, 2002)
    Radio pulsars have played a very important part in the growth of VHE (Very High Energy) gamma-ray astronomy. Apart from their ability to accelerate particles to very high energies, the modest sensitivity of the first ...
  • de Jager, O. C (Astronomical Society of India, 2002)
    This paper explores the potential of present and future ground based gamma-ray telescopes to detect GeV to multi-GeV pulsed emission from EGRET pulsars. Five types of telescopes can in principle detect such emission: The ...
  • Joshi, B. C; Lyne, A. G; Kramer, M (Astronomical Society of India, 2003)
    High time resolution studies of pulsars require specialized instrumentation to counter the degradation in the quality and time resolution of their radio signals due to dispersion in the inter-stellar medium. The availability ...
  • Balasubramanyam, R (Astronomical Society of India, 2003)
    The submillimeter waveband (3 to 0.3 mm) is important for photometric and spectroscopic studies of the high redshift Universe and of the deeply embedded star forming regions in our and nearby galaxies. The upcoming Atacama ...
  • Rangarajan, K. E; Varghese, B. A (Astronomical Society of India, 2003)
    As an important tool of atmospheric remote sensing, microwave radiometers are used for temperature profiling and vapor and liquid column measurements. In addition, ice water path can be retrieved using radiometer observations. ...
  • Krishna, G; Wiita, P. J (Astronomical Society of India, 2003)
    During the `quasar era' at z ~ 2 - 3, radio galaxies had a much higher co-moving density; however, such sources are only detectable for small fractions of their active lifetimes, thanks to expansion losses and inverse ...
  • Mangalam, A (Astronomical Society of India, 2003)
    Supermassive disks are thought to be precursors of supermassive black holes that are believed to power quasars and exist at centers of galaxies. Formation scenarios of such disks are reviewed and it is argued that gas ...
  • Kulkarni, V. P (Astronomical Society of India, 2003)
    A unique tool to investigate distant young galaxies is to study the absorption lines they produce in the spectra of background quasars. The damped Lymanalpha (DLA) quasar absorption line systems allow us to empirically ...
  • Panchapakesan, N (Astronomical Society of India, 2003)
    Magnetars are neutron stars in which a decaying high magnetic field is the source of energy production. The suggestion that magnetars are the dominant source of energy for soft gamma repeaters and anomalous x-ray pulsars ...
  • 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 ...
  • Banerjee, D. P. K; Ashok, N. M (Astronomical Society of India, 2003)
    Near - IR spectroscopic and photometric observations of the eruptive variables V838 Mon and V445 Puppis in the J H K bands are reported. These objects erupted in nova-like explosions but evolved into rather unique and ...
  • Pandey, A. K (Astronomical Society of India, 2003)
    Observational evidences indicate that the formation of open star clusters has been efficient throughout the life of our Galaxy. As a consequence, we find open clusters with ages ranging from a few Myr to few Gyr. This makes ...
  • Mukherjee, R (Astronomical Society of India, 2002)
    High energy astronomy above 30 MeV received a significant impetus from the observations of EGRET (Energetic Gamma-Ray Experiment Telescope) on board the Compton Gamma Ray Observatory (CGRO). Until June 2000, when CGRO was ...

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