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  • Formation of a binary in the general three-body problem 
    Bhatnagar, K. B (Astronomical Society of India, 1990)
    This paper reviews the role of triple encounters in the evolution of stellar systems. If a symmetric triple collision is perturbed, a family of asymmetric triple close approaches with arbitrary escape velocities and with ...
  • Formation of a proto-quasar from accretion flows in a halo 
    Mangalam, A (E D P Sciences, 2001-12)
    We present a detailed model for the formation of massive objects at the centers of galaxies. The effects of supernovae heating and the conditions of gas loss are revisited. The escape time of the gas is compared with the ...
  • Formation of largescale structures in the universe by inverse cascade: cosmosynergetics 
    Krishan, V; Sivaram, C (Nova Science Publishers Inc, 1993)
  • Formation of Spectral Lines with the Redistribution Function R1 along the line of Sight 
    Peraiah, A (Indian Institute of Astrophysics, Bangalore, 1981)
    We studied the formation of spectral lines at infinity with the redistribution function R1. The radial optical depths considered are 5, 5, 10, 50 and 100. A linear law of velocity is assumed in these calculations. Profiles ...
  • Formation of the Hydrogen Lyman α Line in Expanding Spherical Nebulae with Dust 
    Peraiah, A; Wehrse, R (European Southern Observatory, 1978-11)
    The radiation field in the hydrogen Ly α line is calculated for a dust filled spherical gaseous nebula. It is assumed that the nebula with a ratio of inner to outer radius of 3.3 has an optical depth at the line center of ...
  • Forming supermassive black holes like J1342+0928 (invoking dark matter) in early universe 
    Sivaram, C; Arun, K; Kiren, O. V (Springer, 2018-02)
    Recent discovery of J1342+0928 using data from the WISE telescope and ground based surveys indicate presence of a supermassive black hole (SMBH) having a mass of 800 million solar mass at a redshift of about 7.6. This imply ...
  • Forty Hypervelocity Stars from Gaia DR3 
    Parthasarathy, M (American Astronomical Society, 2024-04)
    Forty hypervelocity stars (HVS) are detected from a search for HVS in Gaia DR3 data whose G magnitudes are less than 17.0 and radial velocities are more +400 km s‑1. The Gaia DR3 astrophysical parameters and spectra indicate ...
  • Forward modeling of propagating slow waves in coronal loops and their frequency-dependent damping 
    Mandal, Sudip; Magyar, N; Yuan, D; Van Doorsselaere, T; Banerjee, D (IOP Publishing, 2016-03)
    Propagating slow waves in coronal loops exhibit a damping that depends upon the frequency of the waves. In this study we aim to investigate the relationship of the damping length ( L d ) with the frequency of the ...
  • Forward modeling of standing slow modes in flaring coronal loops 
    Yuan, D; Van Doorsselaere, T; Banerjee, D; Antolin, P (IOP Publishing, 2015-07-01)
    Standing slow-mode waves in hot flaring loops are exclusively observed in spectrometers and are used to diagnose the magnetic field strength and temperature of the loop structure. Owing to the lack of spatial information, ...
  • Forward-scattering Hanle effect in the solar Ca i 4227 Å line 
    Frisch, H; Anusha, L. S; Bianda, M; Holzreuter, R; Nagendra, K. N; Ramelli, R; Sampoorna, M; Smitha, H. N; Stenflo, J. O (Cambridge University Press, 2012-06)
    High sensitivity spectropolarimetric observations of the four Stokes parameters of the solar Ca i 4227 Å line have been performed in October 2010 at IRSOL with the ZIMPOL polarimeter, near the disk center, outside an active ...
  • Fossil magnetic fields of the sun and stars 
    Hiremath, K. M; Gokhale, M. H (Astronomical Society of India, 2000)
    Using helioseismologically inferred internal rotation given by Dziembowski et al., 1989, in the previous work, we (Hiremath and Gokhale 1995, Hiremath 1995) modelled the steady (fossil) part of the poloidal magnetic field ...
  • Four hundredth anniversary of Kepler’s supernova 
    Vishwanath, P. R (Indian Academy of Sciences, 2004-10)
  • Four years of starspot evolution on an active F-type ultra-fast rotator KIC 6791060 
    Karmakar, Subhajeet; Pandey, J. C; Savanov, Igor S; Raj, A; Dmitrienko, E. S; Pakhomov, Yurij; Sahu, D. K (Cambridge University Press, 2018-02)
    Using the data obtained from Kepler satellite, we have analyzed an F-type ultra-fast rotator KIC 6791060. We derive a rotational period of 0.34365±0.00004 d. Multiple periodicity with a period separation of ∼0.00016 d was ...
  • Four-component relativistic state-specific multireference perturbation theory with a simplified treatment of static correlation 
    Ghosh, A; Sinha Ray, Suvonil; Chaudhuri, R. K; Chattopadhyay, Sudip (American Chemical Society, 2017-02-23)
    The relativistic multireference (MR) perturbative approach is one of the most successful tools for the description of computationally demanding molecular systems of heavy elements. We present here the ground state dissociation ...
  • Four-component relativistic state-specific multireference perturbation theory with a simplified treatment of static correlation 
    Ghosh, A; Sinha Ray, Suvonil; Chaudhuri, R. K; Chattopadhyay, Sudip (American Chemical Society, 2017-02-23)
    The relativistic multireference (MR) perturbative approach is one of the most successful tools for the description of computationally demanding molecular systems of heavy elements. We present here the ground state dissociation ...
  • Fourier smoothing of digital photographic spectra 
    Anupama, G. C (Astronomical Society of India, 1990-03)
    Fourier methods of smoothing one-dimensional data are discussed with particular reference to digital photographic spectra. Data smoothed using lowpass filters with different cut-off frequencies are intercompared. A method ...
  • FPGA Based ASM implementation for CCD Camera Controller 
    Srinivasan, R; Anupama, K; Suneeta; Saha, S. K; Rao, A (MacMillan Publishers Ind. Ltd, 2009)
    A general purpose CCD controller that can address any CCD, has been developed at the Indian Institute of Astrophysics. It is based on a Digital Signal Processor (DSP) chip, Motorola DSP 56002 for implementing essential ...
  • FPGA based Digital Backend System for Low Frequency Radio Observations 
    Sarpotdar, Mayuresh N (Indian Institute of Astrophysics, 2013-08)
    Radio Astronomy involves digital systems for processing and analyzing the celestial radio signals received by the radio antennas. In recent days, Field Programmable Gate Arrays (FPGAs) are used for digital signal processing ...
  • FR Cnc - A Young Spotted Star 
    Pandey, J. C (Astronomical Society of India, 2003)
    Optical photometric and spectroscopic studies of the star FR Cnc = BD + 16 1753 have been carried out during the years 2001 - 2002. The star is photometrically variable with a mean period of 0d.8271 ± 0.0002. The rapid ...
  • FR Cnc revisited: photometry, polarimetry and spectroscopy 
    Golovin, A; Galvez-Ortiz, M. C; Hernan-Obispo, M; Andreev, M; Barnes, J. R; Montes, D; Pavlenko, E; Pandey, J. C; Martinez-Arnaiz, R; Medhi, B. J; Parihar, P. S; Henden, A; Sergeev, A; Zaitsev, S. V; Karpov, N (Wiley-Blackwell, 2012-03)
    This paper is part of a multiwavelength study aimed at using complementary photometric, polarimetric and spectroscopic data to achieve an understanding of the activity process in late-type stars. Here, we present the ...

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