activity
19982019
most citedRevival of the magnetar PSR J1622-4950: observations with MeerKAT, Parkes, XMM-Newton, Swift, Chandra, and NuSTAR

161 citations · 1.1k across the 32 of their papers we have counts for

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16 papers · 1 filter

astro-ph2007★ 61 cited

Sub-millimeter Observations of Giant Molecular Clouds in the Large Magellanic Cloud: Temperature and Density as Determined from J=3-2 and J=1-0 transitions of CO

T. Minamidani, N. Mizuno, Y. Mizuno +26

We have carried out sub-mm 12CO(J=3-2) observations of 6 giant molecular clouds (GMCs) in the Large Magellanic Cloud (LMC) with the ASTE 10m sub-mm telescope at a spatial resolutio…

astro-ph2007★ 5 cited

Upper limits to the water abundance in starburst galaxies

C. D. Wilson, R. S. Booth, A. O. H. Oloffson +11

We have searched for emission from the 557 GHz ortho-water line in the interstellar medium of six nearby starburst galaxies. We used the Odin satellite to observe the 1_10-1_01 tra…

astro-ph2007★ 142 cited

Molecular oxygen in the rho Ophiuchi cloud

B. Larsson, R. Liseau, L. Pagani +56

Molecular oxygen, O2 has been expected historically to be an abundant component of the chemical species in molecular clouds and, as such, an important coolant of the dense interste…

astro-ph2006★ 23 cited

A general catalogue of 6.7GHz methanol masers II: statistical analysis

Michele R. Pestalozzi, A. Chrysostomou, J. Collett +3

Context: Methanol masers at 6.7GHz are recognised markers of high-mass star formation regions. The study of their distribution in the Galaxy gives important insights into the star…

astro-ph2005★ 9 cited

Searching for O in the SMC:Constraints on Oxygen Chemistry at Low Metallicities

C. D. Wilson, A. O. H. Olofsson, L. Pagani +5

We present a 39 h integration with the Odin satellite on the ground-state 118.75 GHz line of O2 towards the region of strongest molecular emission in the Small Magellanic Cloud. Ou…

astro-ph2004★ 4 cited

Towards the Event Horizon - The Vicinity of AGN at Micro-Arcsecond Resolution

T. P. Krichbaum, D. A. Graham, W. Alef +18

We summarize the present status of VLBI experiments at 3 mm (86 GHz), 2 mm (129-150 GHz) and 1.3 mm (215-230 GHz). We present and discuss a new 3 mm VLBI map of M87 (Virgo A), whic…