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20012022
most citedEvidence for a developing gap in a 10 Myr old protoplanetary disk

560 citations · 4k across the 73 of their papers we have counts for

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18 papers · 1 filter

astro-ph2008

High velocity water maser emission from the Post-AGB star OH 009.1-0.4

A. J. Walsh, S. L. Breen, I. Bains +1

Observations of HO masers towards the post-AGB star and water fountain source OH 009.1--0.4 were made as part of HOPS (The HO southern galactic Plane Survey), with the Mopr…

astro-ph2008★ 53 cited

Physical and chemical conditions in methanol maser selected hot-cores and UCHII regions

C. R. Purcell, S. N. Longmore, M. G. Burton +4

We present the results of a targeted 3-mm spectral line survey towards the eighty-three 6.67 GHz methanol maser selected star forming clumps observed by Purcell et al. 2006. In add…

astro-ph2008★ 175 cited

The 6-GHz Multibeam Maser Survey I. Techniques

J. A. Green, J. L. Caswell, G. A. Fuller +22

A new 7-beam 6-7 GHz receiver has been built to survey the Galaxy and the Magellanic Clouds for newly forming high-mass stars that are pinpointed by strong methanol maser emission…

astro-ph2008★ 39 cited

A Pilot Survey for the HO Southern Galactic Plane Survey (HOPS)

Andrew J. Walsh, Nadia Lo, Michael G. Burton +5

We describe observations with the Mopra radiotelescope designed to assess the feasibility of the HO maser southern Galactic plane survey (HOPS). We mapped two one-square-degree…

astro-ph2008

Cyanopolyynes and sulphur bearing species in hot cores: Chemical and line excitation models

J. F. Chapman, M. Wardle, T. J. Millar +2

We present results from a time dependent gas phase chemical model of a hot core based on the physical conditions of G305.2+0.2. While the cyanopolyyne HC_3N has been observed in ho…

astro-ph2008★ 74 cited

Spectral imaging of the Sagittarius B2 region in multiple 3-mm molecular lines with the Mopra telescope

P. A. Jones, M. G. Burton, M. R. Cunningham +6

Using the Mopra telescope, we have undertaken a 3-mm spectral-line imaging survey of a 5 x 5 arcmin^2 area around Sgr B2. We covered almost the complete spectral the range from 81.…