Browsing by Author "Omar, A."

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  • Jaiswal, S.; Omar, A. (Indian Academy of Sciences, 2013)
    The Devasthal Fast Optical Telescope (DFOT) is a 1.3 meter aperture optical telescope, recently installed at Devasthal, Nainital. We present here the first results using an Hα filter with this telescope on a Wolf–Rayet ...
  • Omar, A.; Dwarakanath, K. S. (2005)
    TThe GMRT H I 21cm-line observations of galaxies in the Eri- danus group are presented. The Eridanus group, at a distance of ∼ 23 Mpc, is a loose group of ∼ 200 galaxies. The group extends to more than 10 Mpc in ...
  • Omar, A.; Dwarakanath, K. S. (2005)
    The HI content of galaxies in the Eridanus group is studied using the GMRT observations and the HIPASS data. A significant HI deficiency up to a factor of 2–3 is observed in galaxies in the high galaxy density regions. The ...
  • Haarlem, M. P. van, et al.; Omar, A. (ESO, 2013)
    LOFAR, the LOw-Frequency ARray, is a new-generation radio interferometer constructed in the north of the Netherlands and across europe. Utilizing a novel phased-array design, LOFAR covers the largely unexplored low-frequency ...
  • Sagar, R.; Omar, A.; Kumar, Brijesh; Gopinathan, M.; Pandey, S. B.; Bangia, T.; Pant, J.; Shukla, V.; Yadava, S. (2011)
    A modern Ritchey-Chretein Cassegrain 130-cm diameter optical telescope has been successfully installed at Devasthal, Nainital in the central Himalayan region. This location was chosen after carrying out extensive site ...
  • Sagar, R.; Kumar, Brijesh; Omar, A.; Pandey, A. K. (2012)
    Devasthal, located in the Kumaun region of Himalayas is emerging as one of the best optical astronomy site in the continent. The minimum recorded ground level atmospheric seeing at the site is 0.”6 with median value at ...
  • Sagar, R.; Kumar, Brijesh; Omar, A.; Joshi, Y. C. (ASI, 2012)
    The Devasthal Observatory, located at about 2450 m height above sea level in the central Himalayas, operates a 1.3-m optical tele- scope, commissioned in the year 2010 and building another 3.6-m optical telescope to be ...
  • Angiras, R. A.; Jog, C. J.; Omar, A.; Dwarakanath, K. S. (2006)
    The H I surface density maps for a sample of 18 galaxies in the Eridanus group are Fourier analysed. This analysis gives the radial variation of the lopsidedness in the H I spatial distribution. The lopsidedness is ...
  • Omar, A. (CURRENT SCIENCE, 2011)
    The Magnus effect introduced near the turbulent boundary layer in the flow of rotating disk galaxies in the intergalactic medium (IGM) is discussed. The Magnus effect is expected to develop an extra pressure on the outer ...
  • Omar, A.; Dwarakanath, K. S. (2005)
    The Eridanus galaxies follow the well-known radio–FIR correlation. The majority (70%) of these galaxies have their star formation rates below that of the Milky Way. The galaxies that have a significant excess of radio ...
  • Omar, A.; Dwarakanath, K. S. (2006)
    The Tully–Fisher (TF) or the luminosity–linewidth relations of the galaxies in the Eridanus group are constructed using the HI rotation curves and the luminosities in the optical and in the near-infrared bands. The slopes ...

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