Aryabhatta Research Institute of Observational Sciences: Recent submissions

  • Unknown author (IOP, 2011-09)
    We present proper motions, radial velocities, and a photometric study of the Galactic open cluster NGC 7380, which is associated with prominent emission nebulosity and dark molecular clouds. On the basis of the sample of ...
  • Ojha, D. K. (IOP, 2011)
    We present results on the star formation activity of an optically obscured region containing an embedded cluster (S255-IR) and molecular gas between two evolved H II regions, S255 and S257. We have studied the complex using ...
  • Dumka, U. C.; Moorthy, K. K.; Tripathi, S. N.; Hegde, P.; Sagar, Ram (Science Direct, 2011)
    Altitude variations of the mass concentration of black carbon, number concentration of composite aerosols are examined along with the columnar spectral aerosol optical depths using state of the art instruments and the ...
  • Joshi, S.; Chakradhari, S. Joshi (Adv. Geo., 2011)
    The Sun, solar-like oscillators, δ-Scuti and roAp stars are few examples of the main-sequence pulsating stars for which the quantitative measurements of the internal structure parameters have been derived from their ...
  • Srivastava, A. K.; Kumar, Pankaj; Zaqarashvili, T. V.; Filippov, B. P.; Uddin, W. (Adv. Geo., 2011)
    We study the active region NOAA 10960, which produces two flare events (B5.0, M8.9) on 04 June 2007. We find the observational signature of right handed helical twists in the loop system associated with this active region. ...
  • Kumar, M.; Dwived, B. N.; Srivastava, A. K. (Adv. Geo., 2011)
    We analyze the temporal image data of the on-disk coronal hole as observed on 31 March 2007 by the XRT/Hinode telescope and Al-poly filter. We choose this temporal image data of 30 s cadence from 11:34:48 UT to 14:19:35 ...
  • Pandey, J. C.; Srivastava, A. K. (Adv. Geo., 2011)
    Using data from observations made with XMM-Newton, we present an X-ray analysis of two flares observed in ξ Boo. The flare loop parameters are derived using various loop models including state-of-the-art hydrodynamic flare ...
  • Pant, V.; Singh, D.; Kamra, A. K. (2011)
    Measurements of the concentration and size distribution of the atmospheric aerosol particles in the size range of 0.003–20 μm diameter have been made at Maitri (70°45′52″S, 11°44′03″E) during January–February, 2005. The ...
  • Murawski, K.; Srivastava, A. K.; McLaughlin, J. A.; Oliver, R. (2013)
    We investigate the excitation of magnetoacoustic–gravity waves generated from localized pulses in the gas pressure as well as in the vertical component of velocity. These pulses are initially launched at the top of the ...
  • Gopal-Krishna; Goyal, A.; Joshi, S.; Karthick, C.; Sagar, R.; Wiita, P. J.; Anupama, G. C.; Sahu, D. K. (2011)
    In this first systematic attempt to characterize the intranight optical variability (INOV) of TeVdetected blazars, we have monitored a well-defined set of nine TeV blazars on total 26 nights during 2004–10. In this R- or ...
  • Lee, S.; Ryu, D.; Chattopadhyay, I. (2011)
    We investigated the instability of advective accretion flow as a consequence of angular momentum transfer in one-dimensional, quasi-spherical transonic accretion flow around a non-rotating black hole. The code is designed to ...
  • Rani, B.; Gupta, A. C.; Wiita, P. J. (2011)
    The emission from blazars is known to be variable at all wavelengths.The flux variability is often accompanied by spectral changes. Spectral energy distribution (SED) changes must be associated with changes in the spectra ...
  • Gupta, A. C. (2011)
    It is well established that the blazars show flux variations in the complete electromagnetic (EM) spectrum on all possible time scales ranging from a few tens of minutes to several years. Here we report the review of ...
  • Mohan, P.; Mangalam, A.; Chand, H.; Gupta, A. C. (2011)
    We have developed analysis tools to search for quasi periodic oscillations in light curves from active galactic nuclei, using the following time series techniques: Wavelets, periodogram, Lomb–Scargle periodogram, structure ...
  • Chauhan, N.; Pandey, A. K.; Ogura, K.; Jose, J.; Ojha, D. K.; Samal, M. R.; Mito, H. (2011)
    The aim of this paper is to present the results of photometric investigations of the central cluster of the W5 E HII region as well as a follow-up study of the triggered star formation in and around bright-rimmed clouds ...
  • Joshi, R.; Chand, H.; Gupta, A. C.; Wiita, P. J. (2011)
    We present optical light curves of 19 radio-quiet (RQ) broad absorption line (BAL) quasi-stellar objects (QSOs) and study their rapid variability characteristics. Systematic CCD observations, aided by a careful data ...
  • Kumar, M.; Srivastava, A. K.; Dwivedi, B. N. (2011)
    We analyse the temporal image data of the quiet Sun observed by the X-ray Telescope (XRT) onboard the Hinode spacecraft and Al-poly filter on 2007 March 31.We choose these temporal image data of ∼30 s cadence from 11:34:48 ...
  • Balona, L. A.; Joshi, S.; Joshi, Y. C.; Sagar, R. (2013)
    We present an analysis of stars in the field of the open cluster NGC 6866 (age 650 Myr) using data from the Kepler Input Catalogue (KIC) and time series photometry from the Kepler data base. We identify 31 δ Scuti and 8 γ ...
  • Unknown author (ARIES, Nainital, 2012-09)
  • ARIES (2012-02-12)

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