activity
19982026
most citedThe temperature of the WNM in the Milky Way

41 citations · 164 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2026

The Variability of Radio Stars

Laura N. Driessen, Alex Andersson, Joseph R. Callingham +6

Stellar radio emission is highly variable with stellar flares lasting from milliseconds to hours. For some stars, their flares or bursts can repeat once every couple of hours, whil…

astro-ph.GA2026

LeMMINGs VII: 5 GHz, 50 mas e-MERLIN observations of a statistically complete sample of nearby AGN

D. R. A. Williams-Baldwin, R. D. Baldi, R. J. Beswick +36

We present 5 GHz e-MERLIN radio images at 50 mas resolution of the nuclear regions of the Legacy e-MERLIN Multi-band Imaging of Nearby Galaxies survey (LeMMINGs), the deepest stati…

astro-ph.GA2021★ 24 cited

A study of submillimeter methanol absorption toward PKS1830-211: Excitation, invariance of the proton-electron mass ratio, and systematics

S. Muller, W. Ubachs, K. M. Menten +2

Methanol is an important tracer to probe physical and chemical conditions in the interstellar medium of galaxies. Methanol is also the most sensitive target molecule for probing po…

astro-ph2005★ 36 cited

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…

astro-ph2003★ 40 cited

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…

astro-ph2003★ 23 cited

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…