Publications of Astronomical Society of India: Recent submissions

  • Shelke, R. N; Pande, M. C (Astronomical Society of India, 1984-09)
  • Mohan, V; Pandey, A. K (Astronomical Society of India, 1984-09)
    Photoelectric magnitudes of 26 stars in the field of King 21 have been obtained. The reddening is variable across the cluster. A distance of 1.91 kpc has been estimated for the cluster. It is concluded that the age of the ...
  • Prabhu, T. P (Astronomical Society of India, 1984-06)
  • Bappu, M. K. V; Mekkaden, M. V; Kameswara Rao, N (Astronomical Society of India, 1984-06)
    The Changes in the Ca II K line profile of the F0 supergiant Canopus have been studied from the high dispersion coude spectrograms obtained since 1975. The emission in the core of the line is variable in a timescale of few ...
  • Abhyankar, K. D; Subrahmanyam, P. V (Astronomical Society of India, 1984-06)
    An estimation of the correction for the broadening of the intensity profile of the solar corona caused by atmospheric turbulence, scattering in the photographic emulsion, focusing errors etc, is made from the coronal ...
  • Radhakrishnan, K. R; Abhyankar, K. D; Sarma, M. B. K (Astronomical Society of India, 1984-06)
    Photoelectric observations of the Algol-type eclipsing binary R Canis Majoris during three consequtive observing seasons of 1979-82 gave a total of ten primary minima in each of the V and B passbands and nine in the U ...
  • Sinha, K (Astronomical Society of India, 1984-06)
    Utilizing the KPNO atlas (Brault & Testerman 1972) for the (0-0) band of the Swan system of the C/sub2/ molecules, we determine rotational temperatures T/subrot/, for mu = 1.0 and mu = 0.2. When saturation in the observed ...
  • Jain, Rajmal; Bhatnagar, A; Shelke, R. N (Astronomical Society of India, 1984-06)
    An interesting solar flare occured on 1978 December 20 behind the north-west limb, in the McMath active region no. 15700, as inferred from the observed associated energtic mass ejections, strong x-rays, decimetric and ...
  • Chandra, S (Astronomical Society of India, 1984-06)
    We have investigated the amount of heating due to an external source for some coronal loops and kernels in the line-dipole and the point dipole geometrics under nonstatic conditions. Two forms for the external source are ...
  • Hirata, Ryuko; Kogure, T (Astronomical Society of India, 1984-06)
  • Prabhu, T. P (Astronomical Society of India, 1984-03)
  • Kameswara Rao, N; Vagiswari, A; Louis, C (Astronomical Society of India, 1984-03)
    Father Richard who discovered the binary nature of alpha Centauri from Pondicherry is probably the first person to use a telescope on Indian soil. A brief sketch of his life and astronomical contributions from India are presented.
  • Srivastava, R. K (Astronomical Society of India, 1984-03)
    Evolutionary discussion shows that the possibility of AR Lac being in a semi-detached state of evolution cannot be ruled out. The period variations of AR Lac have been analysed using Biermann & Hall's (1973) model for a ...
  • Sinha, K (Astronomical Society of India, 1984-03)
    The recently published values of oscillator strengths for the Phillips bands were checked with those obtainable from the solar spectrum. The results of (1982) Erman et al. based on the assumption of a varying electronic ...
  • Chaubey, U. S; Singh, Mahendra (Astronomical Society of India, 1984-03)
    UBV light curves of the eclipsing binary systems V364 Cas and MM Cas are presented. A total of eight photoelectric times of minimum light for these stars were derived. The UBV photometric data of V364 Cas show that the ...
  • Gehrels, Tom (Astronomical Society of India, 1984-03)
    Planetesimals are intermediate stages, in the kilometer size range between interstellar matter and large bodies such as planets and stars. Planetesimals can still be studied in the form of asteroids although they have been ...
  • Narlikar, J. V (Astronomical Society of India, 1984-03)
  • Singh, J; Rajamohan, R; Raheem, K. C. A (Astronomical Society of India, 1983-12)
    Spectrograms of the inner solar corona were obtained during the 1980 total solar eclipse. Two Ebert-Fastie type spectrographs with circular slits were used to obtain spectra on the east and the west at 1.06 R. These ...
  • Shelke, R. N; Pande, M. C (Astronomical Society of India, 1983-12)
    Interrelationships of filament positions and large scale solar magnetic field structures are examined here. The broad neutral bands seem to be suitable locations for the formation and development of filaments. Filaments ...
  • Markeev, A. K; Formichev, V. V; Chertok, I. M; Bhatnagar, A; Jian, R. M; Shelke, R. N; Bhonsle, R. V (Astronomical Society of India, 1983-12)
    The observations of the 1980 March 28, 2B flare in optical, radio microwave and metric and x-ray wavelengths are presented. In the dynamic radio spectrum, unusual and rare U-shaped type II radio bursts associated with this ...

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