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Results 1321-1330 of 1781 (Search time: 0.018 seconds).
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Issue DateTitleAuthor(s)Citation
29-May-1990A modified algorithm for CLEANing wide-field maps with extended structures.Dwarakanath, K S; Deshpande, A A; Shankar, Udaya NJournal of Astrophysics and Astronomy, 1990, Vol. 11, p311-322.
1984On the supernova remnants produced by pulsars.Srinivasan, G; Bhattacharya, D; Dwarakanath, K SJournal of Astrophysics and Astronomy, 1984, Vol. 5, p403 -423.
9-Jul-1991Low-frequency observations of the Vela supernova remnant and their implicationsDwarakanath, K SJournal of Astrophysics and Astronomy, 1991, Vol. 12, p199-211.
20-Jun-1982On the implications of the radio and x-ray pulsar in the supernova remnant MSH 15-52Srinivasan, G; Dwarakanath, K S; Radhakrishnan, VCurrent Science, 1982, Vol. 51, p596-599.
1991modified CLEAN algorithm for wide field images with extended structuresDwarakanath, K S; Deshpande, A A; Shankar, Udaya NASP conference Series Vol.19,p.242
2004A high galactic latitude HI 21cm-line absorption survey using the GMRT: I. observations and spectraMohan, Rekhesh; Dwarakanath, K S; Srinivasan, GJournal of Astrophysics and Astronomy, 2004, Vol. 25, p143-183.
Nov-2002GMRT and VLA observations of H I and OH from the Seyfert galaxy Mrk 1Omar, A; Dwarakanath, K S; Rupen, M; Anantharamaiah, K RAstronomy and Astrophysics, 2002, Vol.394, p405-414
2004A high galactic latitude HI 21 cm-line absorption survey using the GMRT: II. Results and interpretationMohan, Rekhesh; Dwarakanath, K S; Srinivasan, GJournal of Astrophysics and Astronomy, 2004, Vol. 25, p185-202.
2003GMRT detection of HI 21 cm associated absorption towards the z = 1.2 red quasar 3C 190Ishwara-Chandra, C H; Dwarakanath, K S; Anantharamaiah, K RJournal of Astrophysics and Astronomy, 2003, Vol. 24, p37-43.
Jun-2003An HI survey of clusters in the local universeVan Gorkom, J H; Bravo-Alfaro, H; Dwarakanath, K S; Guhathakurta, P; Poggianti, B M; Schiminovich, D; Valluri, M; Verheijen, Marc; Wilcots, E; Zabludoff, AAstrophysics and Space Science, 2003, Vol.285, p219-224

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