41 citations · 164 across the 8 of their papers we have counts for
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Outflows from young objects observed with the ISO-LWS I. Fine structure lines [O I] 63, [O I]145 and [C II]157 micron
R. Liseau, K. Justtanont, A. G. G. M. Tielens
Far infrared fine structure line data from the ISO archive have been extracted for several hundred YSOs and their outflows, including molecular (CO) outflows, optical jets and Herb…
Detection of OH and wide HI absorption toward B0218+357
N. Kanekar, J. N. Chengalur, A. G. de Bruyn +1
We present deep GMRT OH and WSRT HI absorption spectra of the gravitational lens toward B0218+357. Both the 1665 MHz and 1667 MHz OH lines are clearly detected for the…
The use of OH "main" lines to constrain the variation of fundamental constants
Nissim Kanekar, Jayaram N Chengalur
We describe a new technique to measure variations in the fundamental parameters and , using the sum of the frequencies of cm-wave OH ``main'' lines. The techn…
The temperature of the WNM in the Milky Way
Nissim Kanekar, Ravi Subrahmanyan, Jayaram N. Chengalur +1
We report high spectral resolution Australia Telescope Compact Array HI 21 cm observations resulting in the detection of the warm neutral medium (WNM) of the Galaxy in absorption a…
Upper Limits on the Pulsed Radio Emission from the Geminga Pulsar at 35 & 327 MHz
R. Ramachandran, A. A. Deshpande, C. Indrani
We report here our observations at 35 MHz and 327 MHz made in the direction of the Gamma Ray pulsar Geminga. Based on the observed absence of any significant pulsed emission from t…