| Issue Date | Title | Author(s) | Citation |
Dec-2006 | Limits on the AGN activities in X-ray-underluminous galaxy groups | Dwarakanath, K.S.; Nath, Biman B. | Astrophysical Journal, 2006, Vol.653, pL9-L12 |
9-Jul-1991 | Low-frequency observations of the Vela supernova remnant and their implications | Dwarakanath, K.S. | Journal of Astrophysics and Astronomy, 1991, Vol. 12, p199-211. |
29-May-1990 | A modified algorithm for CLEANing wide-field maps with extended structures. | Dwarakanath, K.S.; Deshpande, A.A.; Udaya Shankar, N. | Journal of Astrophysics and Astronomy, 1990, Vol. 11, p311-322. |
1991 | modified CLEAN algorithm for wide field images with extended structures | Dwarakanath, K.S.; Deshpande, A.A.; Udaya Shankar, N. | ASP conference Series Vol.19,p.242 |
Jan-2012 | Multi-frequency studies of radio relics in the galaxy clusters A4038, A1664, and A786 | Kale, Ruta; Dwarakanath, K.S. | Astrophysical Journal, 2012, Vol.744, p1 |
10-Nov-1998 | Multiwavelength observation of a new black hole candidate: EXS 1737.9-2952 | Durouchoux, Ph.; Vilhu, O.; Corbel, S.; Wallyn, P.; Dwarakanath, K.S.; Huovelin, J.; Anantharamaiah, K.R.; Grindlay, J.; Chapuis, C.; Park, Y.S.; Bally, J.; Mahoney, W. | The Astrophysical Journal, 1998, Vol.507, p.781-793 |
Mar-1982 | A new look at SNR birthrate and evidence for a predominantly low-density interstellar medium | Srinivasan, G.; Dwarakanath, K.S. | Bulletin of the Astronomical Society of India, 1982, Vol.10, p48 |
1982 | A new look at the birthrate of supernova remnants | Srinivasan, G.; Dwarakanath, K.S. | Journal of Astrophysics and Astronomy, 1982, Vol. 3, p351-361. |
Mar-1981 | Observations and interpretation of the slowly varying component of solar radio emission at decameter wavelengths | Sastry, C.V.; Dwarakanath, K.S.; Shevgaonkar, R.K.; Krishan, V. | Bulletin of the Astronomical Society of India, 1981, Vol.9, p75-76 |
Oct-1981 | Observations and interpretation of the slowly varying component of solar radio emission at decameter wavelengths | Sastry, Ch.V.; Dwarakanath, K.S.; Shevgaonkar, R.K.; Krishan, Vinod | Solar Physics, 1981, Vol.73, p363-377 |
1982 | Observations of the supernova remnants HB 9 and IC 443 at 34.5 MHz | Dwarakanath, K.S.; Shevgaonkar, R.K.; Sastry, Ch.V. | Journal of Astrophysics and Astronomy, 1982, Vol. 3, p207-216. |
Jun-1982 | Observations of the supernova remnants HB 9 and IC 443 at 34.5 MHz | Dwarakanath, K.S.; Shevgaonkar, R.K.; Sastry, C.H. | Journal of Astrophysics and Astronomy, 1982, Vol.3, p207 |
Aug-1999 | On the different radio source populations in the Butcher-Oemler clusters Abell 2125 and 2645 | Dwarakanath, K.S.; Owen, F.N. | The Astronomical Journal, 1999, Vol.118, p.625-632 |
20-Jun-1982 | On the implications of the radio and x-ray pulsar in the supernova remnant MSH 15-52 | Srinivasan, G.; Dwarakanath, K.S.; Radhakrishnan, V. | Current Science, 1982, Vol. 51, p596-599. |
2004 | On the origin of the wide HI absorption line towards Sgr A* | Dwarakanath, K.S.; Goss, W.M.; Zhao, J.H.; Lang, Cornelia C. | Journal of Astrophysics and Astronomy, 2004, Vol. 25, p129-141. |
1984 | On the supernova remnants produced by pulsars. | Srinivasan, G.; Bhattacharya, D.; Dwarakanath, K.S. | Journal of Astrophysics and Astronomy, 1984, Vol. 5, p403 -423. |
Jul-2006 | Origin of disc lopsidedness in the Eridanus group of galaxies | Angiras, R.A.; Jog, C.J.; Omar, A.; Dwarakanath, K.S. | Monthly Notices of the Royal Astronomical Society, 2006, Vol.369, p1849-1857 |
Jul-2006 | Origin of disc lopsidedness in the Eridanus group of galaxies | Angiras, R.A.; Jog, C.J.; Omar, A.; Dwarakanath, K.S. | Monthly Notices of the Royal Astronomical Society, 2006 Vol.369, Issue 4, p1849-1857. |
Sep-2009 | Origin of disk lopsidedness in spiral galaxies | Angiras, R.A.; Jog, C.J.; Dwarakanath, K.S.; Omar, A.; Verheijen, M.A.W. | ASP Conference Series, 2009, Vol.407, p79 |
1-Nov-2000 | Power spectrum of the density of cold atomic gas in the galaxy toward Cassiopeia A and Cygnus A | Deshpande, A.A.; Dwarakanath, K.S.; Goss, W.M. | Astrophysical Journal, 2000, Vol.543, p227-234 |
