Research Papers: Recent submissions

  • Maheswar, G.; Sharma, S.; Biman, J. M.; Pandey, A. K.; Bhatt, H. C. (2007)
    Using Hα grism spectroscopy and optical and Two-Micron All-Sky Survey photometry of the fields containing NGC 1893 and two emission nebulae, Sim 129 and Sim 130, we show the presence of a number of Hα and near-infrared ...
  • Kamble, A.; Resmi, L.; Misra, K. (2007-07-20)
    The collapse of a massive star is believed to be the most probable progenitor of a long gamma-ray burst (GRB). Such a star is expected to have its environment modified by the stellar wind. The effect of such a ...
  • Joshi, B.; Manoharan, P. K.; Veronig, A. M.; Pant, P.; Pandey, K. (2007)
    The evolution of an X2.7 solar flare, that occurred in a complex βγ δ magnetic configuration region on 3 November 2003 is discussed by utilizing a multi-wavelength data set. The very first signature of pre-flare coronal ...
  • Goyal, A.; Krishna, G.; Sagar, R.; Anupama, G. C.; Sahu, D. K. (2007)
    Although well established for BL Lac objects and radio-loud quasars, the occurrence of intra-night optical variability (INOV) in radio-quiet quasars is still debated, primarily since only a handful of INOV events with ...
  • Maheswar, G.; Muthu, C.; Sujatha, N. V.; Pandey, G.; Bhatt, H. C.; Rao, N. K.; Murthy, J. (2007)
    We propose to carry out studies on the properties of inter- stellar dust using TAUVEX. Through the multi-band TAUVEX observations, particularly with the use of filters optimized for extinction observations of the 2175 ...
  • Ali, S. S.; Uddin, W.; Chandra, R.; Mary, D. L.; Vršnak, B. (2007)
    The eruption of limb prominence on 21 April 2001 associated with two coronal mass ejections (CMEs) is investigated. Hα images reveal two large-scale eruptions (a promi- nence body and a southern foot-point arch), both ...
  • Tiwari, S. K.; Chaubey, U. S.; Pandey, C. P. (2007-08-17)
  • Pandey, A. K.; Sharma, S.; Upadhyay, K.; Ogura, K.; Sandhu, T. S.; Mito, H.; Sagar, R. (2007-06-25)
    We present CCD photometry in a wide field around two open clusters, NGC 1912 and NGC 1907. The stellar surface density profiles indicate that the radii of the clusters NGC 1912 and NGC 1907 are ~14́ and ~6́respectively. ...
  • Sharma, S.; Pandey, A. K.; Ojha, D. K.; Chen, W. P.; Ghosh, S. K.; Bhatt, B. C.; Maheswar, G.; Sagar, R. (2007)
    We present a comprehensive multiwavelength study of the star-forming region NGC 1893 to explore the effects of massive stars on low-mass star formation. Using near-infrared colours, slitless spectroscopy and narrow-band ...
  • Misra, K.; Pooley, D.; Chandra, P.; Bhattacharya, D.; Ray, A. K.; Sagar, R.; Lewin, W. H. G. (2007)
    We present X-ray, broad-band optical and low-frequency radio observations of the bright type IIP supernova SN 2004et. The Chandra X-ray Observatory observed the supernova at three epochs, and the optical coverage spans ...
  • Kaur, R.; Paul, B.; Kumar, B.; Sagar, R. (2008-04-01)
    We report here a study of the long-term properties of quasiperiodic oscillations (QPOs) in an unusual accreting X-ray pulsar, 4U 1626À67. This is a unique accretion-powered X-ray pulsar in which we have found the QPOs to ...
  • Sharma, S.; Pandey, A. K.; Ogura, K.; Aoki, T.; Pandey, K.; Sandhu, T. S.; Sagar, R. (2008-05)
    Using homogeneous CCD photometric data from the 105 cm Kiso Schmidt telescope covering a 50' × 50' field, we study the mass functions (MFs) of nine open clusters. The ages and Galactocentric distances of the target ...
  • Jose, J.; Pandey, A. K.; Ojha, D. K.; Ogura, K.; Chen, W. P.; Bhatt, B. C.; Ghosh, S. K.; Minto, H.; Maheswar, G.; Sharma, S. (2008)
    We present UBVIc CCD photometry of the young open cluster Stock 8 with the aim of studying its basic properties such as the amount of interstellar extinction, distance, age, stellar contents and initial mass function ...
  • Pandey, A. K.; Sharma, S.; Ogura, K.; Ojha, D. K.; Chen, W. P.; Bhatt, B. C.; Ghosh, S. K. (2008)
    We present UBV Ic CCD photometry of the young open cluster Be 59 with the aim to study the star formation scenario in the cluster. The radial extent of the cluster is found to be ∼10 arcmin (2.9 pc). The interstellar ...
  • Uddin, W.; Joshi, B.; Kumar, T. S.; Sharma, S.; Sagar, R. (2007-10-10)
    We report preliminary results on short-period oscillations in the corona and changes in the earth's atmospheric parameters, observed during a total solar eclipse of 29 March 2006 from Manavgat, Turkey
  • Bagchi, J.; Gopal-Krishna; Krause, M.; Joshi, S. (2007-12-01)
    We report the discovery of a very unusual, highly asymmetric radio galaxy whose radio jet, the largest yet detected, emits strongly polarized synchrotron radiation and can be traced all the way from the galactic ...
  • Sagar, R. (2007)
  • Samal, M. R.; Pandey, A. K.; Ojha, D. K.; Ghosh, S. K.; Kulkarni, V. K.; Bhatt, B. C. (2007-12-10)
    We present the observational results of Galactic H II region Sh 2-294, using optical photometry, narrowband imaging, and radio continuum mapping at 1280 MHz, together with archival data from the 2MASS, MSX, and IRAS surveys. ...
  • Sagar, R. (2007)
    The scientific development in the field of observational astronomy in India has been quite significant in the recent past. India has three 2-meter class optical and near infrared telescopes. These telescopes are mainly ...
  • Castro-Tirado, A. J., ...et al. (including Mishra, K. & Sagar, R.) (2007)
    We present multiwavelength (X-ray/optical/near-infrared/millimetre) observations of GRB 051022 between 2.5 h and ∼1.15 yr after the event. It is the most intense gamma-ray burst (∼10-⁴ erg cm-² ) detected by HETE-2, with ...

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