activity
19992009
most citedA multifrequency study of giant radio sources-II. Spectral ageing analysis of the lobes of selected sources

78 citations · 388 across the 15 of their papers we have counts for

collaborators

10 papers

astro-ph2007

A 610-MHz Galactic Plane Pulsar Search with the Giant Meterwave Radio Telescope

B. C. Joshi, M. A. McLaughlin, M. Kramer +5

We report on the discovery of three new pulsars in the first blind survey of the north Galactic plane (45 < l < 135 ; |b| < 1) with the Giant Meterwave Radio telescope (GMRT) at an…

astro-ph200719 cited

The effect of Pulse profile evolution on Pulsar Dispersion Measure

Amrit Lal Ahuja, Dipanjan Mitra, Yashwant Gupta

In an earlier paper (Ahuja, et al, 2005), based on simultaneous multi-frequency observations with the Giant Metrewave Radio Telescope (GMRT), we reported the variation of pulsar di…

astro-ph20032 cited

Giant pulses in Millisecond Pulsars

B. C. Joshi, M. Kramer, A. G. Lyne +2

Giant pulses (GPs), occasional individual pulses with an intensity 100 times the average intensity, have been detected in four pulsars todate. Their origin is not well understood,…

astro-ph2001

Low-frequency Carbon Recombination Lines towards HI self-absorption features in the Galactic Plane

D. Anish Roshi, Nimisha G. Kantharia, K. R. Anantharamaiah

A survey of radio recombination lines (RLs) in the Galactic plane ( 332° 89°) near 327 MHz made using the Ooty Radio Telescope (ORT) has detected carbon RLs from all the…

astro-ph2001

Stability of realistic strange stars (RSS)

Siddhartha Bhowmick, Jishnu Dey, Mira Dey +2

A modified version of this paper is under process and with a new title and abstract. Hence, this version of the article is completely withdrawn.

astro-ph2000

Far infrared observations of the southern Galactic star forming complex around IRAS 09002-4732

S. K. Ghosh, B. Mookerjea, T. N. Rengarajan +2

The Galactic star forming region in the southern sky, associated with IRAS 09002-4732 has been mapped simultaneously in two far infrared bands (148 & 209 um), with ~ 1' angular res…