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Results 1311-1320 of 1781 (Search time: 0.01 seconds).
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Issue DateTitleAuthor(s)Citation
Oct-1981Observations and interpretation of the slowly varying component of solar radio emission at decameter wavelengthsSastry, Ch V; Dwarakanath, K S; Shevgaonkar, R K; Krishan, VSolar Physics, 1981, Vol.73, p363-377
Jun-2021Giant Metrewave Radio Telescope Detection of Hi 21 cm Emission from Star-forming Galaxies at z approximate to 1.3Chowdhury, Aditya; Kanekar, Nissim; Das, Barnali; Dwarakanath, K S; Sethi, ShivAstrophysical Journal Letters, 2021, Vol.913, pL24
Jun-1982Observations of the supernova remnants HB 9 and IC 443 at 34.5 MHzDwarakanath, K S; Shevgaonkar, R K; Sastry, Ch VJournal of Astrophysics and Astronomy, 1982, Vol.3, p207
Mar-1981Observations and interpretation of the slowly varying component of solar radio emission at decameter wavelengthsSastry, Ch V; Dwarakanath, K S; Shevgaonkar, R K; Krishan, VBulletin of the Astronomical Society of India, 1981, Vol.9, p75-76
Mar-1982A new look at SNR birthrate and evidence for a predominantly low-density interstellar mediumSrinivasan, G; Dwarakanath, K SBulletin of the Astronomical Society of India, 1982, Vol.10, p48
1982A new look at the birthrate of supernova remnantsSrinivasan, G; Dwarakanath, K SJournal of Astrophysics and Astronomy, 1982, Vol. 3, p351-361.
Mar-1981A study of a supernova remnantDwarakanath, K S; Sastry, Ch VBulletin of the Astronomical Society of India, 1981, Vol.9, p77
29-May-1990A synthesis map of the sky at 34.5 MHz.Dwarakanath, K S; Shankar, Udaya NJournal of Astrophysics and Astronomy, 1990, Vol. 11, p323-410.
1985How often are remnants like the Crab Nebula bornDwarakanath, K S; Srinivasan, GProceedings of the Academy Workshop on Supernovae, their Progenitors and Remnants, October 29-November 2, 1984, Raman Research Institute, Bangalore. Eds., G. Srinivasan, V. Radhakrishnan; Indian Academy of Sciences, Bangalore, 1985, p97-103
1993GRB 930309Beasley, A J; Dwarakanath, K S; Rupen, M P-

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