Publications of Astronomical Society of India: Recent submissions

  • Acharyya, K; Chakrabarti, S. K (Astronomical Society of India, 2005-12)
    We study the efficiency of molecular hydrogen recombination on grain surfaces using both the rate equation (which tracks the average number of species) and the master equation (which tracks the expectation values of the ...
  • Ghanbari, J; Shadmehri, M; Salehi, F (Astronomical Society of India, 2005-12)
    We study the nonlinear dynamics of a warped or twisted accretion disc, in which the viscosity coefficients are assumed to be locally proportional to the rotational velocity (Beta -prescription). Using asymptotic methods ...
  • Mekkaden, M. V; Pukalenthi, S; Muneer, S; Bastian, A. B (Astronomical Society of India, 2005-12)
    We present spectroscopic observations in the region of H alpha and Li I lines of the weak emission T Tauri star V410 Tau obtained over 1999/2000, 2002/2003 and 2003/2004 seasons. The emission strength showed rotational ...
  • Tadross, A. L (Astronomical Society of India, 2005-12)
    A deep photometric analysis in the open star cluster NGC 1883 has been presented here and added to the work of Carraro et al. (2003), which is the only previous work introduced for this cluster. The radius and metallicity ...
  • Ravindra, B (Astronomical Society of India, 2005-09)
    The Sun affects the terrestrial climate and weather as well as near Earth space by its high energy radiation and particle emissions. It is now becoming clear that the solar magnetic field, which controls all the physical ...
  • Manoj, P (Astronomical Society of India, 2005-09)
    In this thesis we have undertaken a detailed study of the evolution of young circumstellar disks from the early pre-main sequence phase to the main sequence phase. We have used several observational diagnostics of the disks ...
  • Mehta, M (Astronomical Society of India, 2005-09)
    Solar rotation continues to be observed by several techniques. We have tried to study coronal rotation using radio observations. Coronal rotation and its variation with height in solar atmosphere are studied. For this, we ...
  • Joshi, S (Astronomical Society of India, 2005-09)
    This thesis is on the framework of the "NainiTal-Cape Survey" programme for searching photometric variability in chemically peculiar stars, initiated in 1997 at the ARIES, NainiTal, India, in collaboration with the South ...
  • Hasan, P (Astronomical Society of India, 2005-09)
    Infrared observations of young star clusters provide vital clues to the star formation process and evolution of stars. This brief report on my thesis gives a brief description of the observations and analysis of the young ...
  • Das, S (Astronomical Society of India, 2005-09)
    Shocks in advective flows around black holes have become es- sential ingredients in explaining wide variety of observed features. We first analytically study the properties of shocks in the special case when viscosity and ...
  • Choudhury, M (Astronomical Society of India, 2005-09)
    Microquasars provide a unique laboratory to study the accretion process in a compact object, coupled to the ejection of matter in the form of jets. In this thesis we provide a phenomenological perspective on the accretion- ...
  • Tandon, S. N (Astronomical Society of India, 2005-09)
  • Chandra, S; Musrif, P. G; Prasad, L (Astronomical Society of India, 2005-09)
    Ionson (1985a) extended his uni¯ed theory of coronal resonance heating having non-resonant (D.C.) and resonant (A.C.) components. Narain and Kumar (1995) calculated heating e±ciency for resonant and non-resonant components ...
  • Venkatakrishnan, P; Sridharan, R; Gupta, S. K (Astronomical Society of India, 2005-09)
    Modern solar telescope designs are different from the conven- tional concept of vacuum telescopes. These new designs are "open" telescopes which try to minimize the temperature difference between various parts of the ...
  • Sharma, S; Sinha, H. S. S (Astronomical Society of India, 2005-06)
    An atmospheric science laboratory was set up at Gurushikhar, in the campus of PRL's Infrared observatory, in 1994. A variety of scientific instruments were housed in the atmospheric science laboratory to explore the Earth's ...
  • Sreekumar, P (Astronomical Society of India, 2005-06)
    Since the advent of the satellite era, X-ray astronomy and UV astronomy have advanced tremendously. The discovery of intense X-ray emission from accreting compact objects has permitted very detailed timing and spectral ...
  • Singal, A. K (Astronomical Society of India, 2005-06)
    Some basic concepts in use for making astronomical observations at radio wavelengths are introduced. In particular the importance of phase information for imaging in radio astronomy is highlighted. Using simple examples ...
  • Shah, R. R. et. al. (Astronomical Society of India, 2005-06)
    The 1.2 m Mt. Abu telescope at Gurushikhar is operated by the Astronomy & Astrophysics Division of Physical Research Laboratory, Ahmed- abad. The evolution of the telescope control system to its present form has been ...
  • George, K; Chandrasekhar, T (Astronomical Society of India, 2005-06)
    We report on the detection at Mt.Abu of H+ 3 molecular ion emissions in the near infrared spectra of the northern auroral zone of Jupiter. These H+3 transitions are of rotational-vibrational origin and are due to the ...
  • Joshi, J. C (Astronomical Society of India, 2005-06)
    The sunlight is scattered by the dust grains present in the coma and tail of comets which makes it visible. The scattered sunlight is characteristically polarized with degree of polarization generally depending upon the ...

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