activity
19972020
most citedThe 6-GHz methanol multibeam maser catalogue I: Galactic Centre region, longitudes 345 to 6

272 citations · 2.6k across the 53 of their papers we have counts for

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Showing 2006Show all

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astro-ph2006★ 27 cited

The JCMT Spectral Legacy Survey

R. Plume, G. A. Fuller, F. Helmich +30

Stars form in the densest, coldest, most quiescent regions of molecular clouds. Molecules provide the only probes which can reveal the dynamics, physics, chemistry and evolution of…

astro-ph2006★ 32 cited

The Water Vapor Abundance in Orion KL Outflows

J. Cernicharo, J. R. Goicoechea, F. Daniel +7

We present the detection and modeling of more than 70 far-IR pure rotational lines of water vapor, including the 18O and 17O isotopologues, towards Orion KL. Observations were perf…

astro-ph2006★ 27 cited

The compact circumstellar material around OH 231.8+4.2

M. Matsuura, O. Chesneau, A. A. Zijlstra +7

We have observed the bipolar post-AGB candidate OH 231.8+4.2, using the mid-infrared interferometer MIDI and the infrared camera with the adaptive optics system NACO on the Very La…

astro-ph2006★ 45 cited

A far-infrared molecular and atomic line survey of the Orion KL region

M. R. Lerate, M. J. Barlow, B. M. Swinyard +8

We have carried out a high spectral resolution line survey towards the Orion Kleinmann-Low (KL) cluster from 44-188 um. The observations were taken with the Long Wavelength Spectro…

astro-ph2006★ 14 cited

A detailed modelling of the chemically rich clumps along the CB3 outflow

Milena Benedettini, Jeremy A. Yates, Serena Viti +1

In order to investigate the origin and the structure of the low velocity, chemically rich clumps observed along the lobes of low- and intermediate-mass outflows, we construct a det…

astro-ph2006★ 33 cited

Far-IR Excited OH Lines from Orion KL Outflows

Javier R. Goicoechea, Jose Cernicharo, Mercedes R. Lerate +6

As part of the first far-IR line survey towards Orion KL, we present the detection of seven new rotationally excited OH Lambda-doublets (at 48, 65, 71, 79, 98 and 115 um). Observat…