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  • Emission from the sub-millisecond pulsar in SN 1987A 
    Sivaram, C; de Sabbata, V (International Cosmic Ray, 1990)
    We consider the production and emission of high energy particles from the sub millisecond pulsar, newly discovered in SN 1987A. We also discuss the emission of very high energy gamma rays and other electromagnetic radiation ...
  • Emission line diagnostics for a coronal condensation 
    Raju, P. K (Astronomical Society of Indian, 1989-09)
    Theoretical line emission rates for the coronal ions Fe X, Fe XI, FE XIII, Fe XIV, Ca XII, Ca XIII, and Ca XV, have been used to obtain various line intensity ratios as a function of electron density and electron temperature. ...
  • An emission line in the solar spectrum near K 
    Evershed, John (Royal Astronomical Society, 1927-03)
  • Emission line star catalogues post-Gaia DR3: A validation of Gaia DR3 data using the LAMOST OBA emission catalogue 
    Shridharan, B; Mathew, B; Bhattacharyya, S; Robin, T; Arun, R; Kartha, S. S; Manoj, P; Nidhi, S; Maheswar, G; Paul, K. T; Narang, M; Himanshu, T (EDP Sciences, 2022-12)
    Aims. Gaia Data Release 3 (DR3) and further releases have the potential to identify and categorise new emission-line stars in the Galaxy. We perform a comprehensive validation of astrophysical parameters from Gaia DR3 ...
  • Emission Line Studies of Wolf Rayet Binaries 
    Shylaja, B. S (Indian Institute of Astrophysics, Bangalore, 1986)
  • Emission lines from nitrogen-like ions and their diagnostic use 
    Raju, P. K; Dwivedi, B. N (Kluwer Academic Publishers, 1990-11)
    Line emissions from nitrogen-like ions NeIV, MgVI, and AlVII have been studied as a diagnostic probe for the emitting regions of astrophysical plasma. Line intensities from these ions have been calculated and compared, in ...
  • Emission lines from X-ray illuminated accretion disc in black hole binaries 
    Mondal, Santanu; Adhikari, Tek P; Singh, Chandra B (Oxford University Press on behalf of the Royal Astronomical Society, 2021-07)
    X-ray flux from the inner hot region around central compact object in a binary system illuminates the upper surface of an accretion disc and it behaves like a corona. This region can be photoionized by the illuminating ...
  • Emission lines of inner corona observed during the total solar eclipse of 1980 February 16 
    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 ...
  • Emission lines on the absorption bands of H and K 
    Evershed, John (Royal Astronomical Society, 1929-04)
  • Emission mechanism of extragalactic X-ray and radio sources 
    Krishan, V (Gordon and Breach Science Publishers, 1983)
    An alternative way of looking at the process of comptonization and the roles of the microwave background radiation density and of the ambient magnetic field in the generation of X-rays on the galactic scale is suggested. ...
  • Emission Spectrum of Hot R CrB star Mv Sgr 
    Kameswara Rao, N; Houziaux, L; Giridhar, S (Indian Academy Sciences, 1990-03)
    The new spectroscopic observation of MV Sgr obtained at ESO in 1987july shows enhanced emission lines of He I , λ 3889, [S II ] λ 4068 relative to the observations discussed by Jeffrey et al. (1988). The presence of [SII] ...
  • Emission-line CCD imaging of three southern symbiotic stars 
    Bhatt, H. C; Sagar, R (Indian Academy of Sciences, 1991-06)
    Symbiotic stars that are strong radio sources and have cool dust emitting in the IR are expected to have extended emission nebulae around them. In order to search for such emission nebulae, CCD imaging of three symbiotic ...
  • Emission-line profiles from expanding envelopes 
    Bappu, M. K. V; Menzel, D. H (University of Chicago Press, 1954-05)
    We have developed a method for calculating the emission-line profiles from an expanding envelope. The method applies to an envelope where the emission intensity varies with latitude. Some typically illustrative cases are ...
  • Emission-line spectra of XX Ophiuchi in 1996 and 1997 
    Goswami, A; Kameswara Rao, N; Lambert, D. L (The Observatory, 2001-04)
  • The emission-line spectrum of the hot R Coronae Borealis star MV SGR 
    Pandey, G; Kameswara Rao, N; Lambert, D. L (Royal Astronomical Society, 1996-10)
    Spectra of MV Sgr obtained at CTIO in 1992 May show many emission lines in the red. Most of the emission lines show two components with a minimum centred at the stellar velocity. Species represented include H, HeI, TiII ...
  • Empirical Determination of Threshold Partial Wave Amplitudes for pp → ppω 
    Ramachandran, G; Balasubramanyam, J; Vidya, M. S; Venkataraya (World Scientific Publishing Company, 2006-08)
    Using the model-independent irreducible tensor approach to ω production in pp collisions, we show theoretically that it is advantageous to measure experimentally the polarization of ω, in addition to the proposed experimental ...
  • Empirical Determination of Threshold Partial Wave Amplitudes in p p --> p p omega 
    Ramachandran, G; Balasubramanyam, J; Vidya, M. S; Venkataraya (World Scientific Publishing Co, 2006-08)
    Using the model independent irreducible tensor approach to omega production in pp collisions, we show theoretically that it is advantageous to measure experimentally the polarization of w, in addition to the proposed ...
  • An empirical relation to estimate host galaxy stellar light from AGN spectra 
    Jalan, Priyanka; Rakshit, Suvendu; Woo, Jong-Jak; Kotilainen, Jari; Stalin, C. S (Oxford University Press on behalf of Royal Astronomical Society, 2023-05)
    Measurement of black hole mass for low-z (z≤ 0.8) Active Galactic Nuclei (AGNs) is difficult due to the strong contribution from host galaxy stellar light necessitating detailed spectral decomposition to estimate the AGN ...
  • Encouraging Scientists 
    The Rotator Bulletin of the Rotary Club of Bangalore (The Rotator Bulletin of the Rotary Club of Bangalore, 1978-04-14)
  • Energetic Solar Particles 
    Biswas, S (Astronomical Society of India, 1975-12)

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