activity
20062008
most citedThe 6-GHz Multibeam Maser Survey I. Techniques

175 citations · 542 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph2008175 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-ph200847 cited

Investigating the transport of angular momentum from young stellar objects: do H2 jets from Class I YSOs rotate?

A. Chrysostomou, F. Bacciotti, B. Nisni +4

In this pilot study, we examine molecular jets from the embedded Class I sources, HH 26 and HH 72, to search, for the first time, for kinematic signatures of jet rotation from youn…

astro-ph200816 cited

Near-Infrared Imaging Polarimetry of Young Stellar Objects in rho-Ophiuchi

A. F. Beckford, P. W. Lucas, A. C. Chrysostomou +1

The results of a near-infrared (J H K LP) imaging linear polarimetry survey of 20 young stellar objects (YSOs) in rho Ophiuchi are presented. The majority of the sources are unreso…

astro-ph2007172 cited

The James Clerk Maxwell Telescope Legacy Survey of Nearby Star-forming Regions in the Gould Belt

D. Ward-Thompson, J. Di Francesco, J. Hatchell +59

This paper describes a James Clerk Maxwell Telescope (JCMT) legacy survey that has been awarded roughly 500 hrs of observing time to be carried out from 2007 to 2009. In this surve…

astro-ph200623 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-ph200682 cited

Spectropolarimetry of the 3.4 micron Feature in the Diffuse ISM toward the Galactic Center Quintuplet Cluster

J. E. Chiar, A. J. Adamson, D. C. B. Whittet +6

Aliphatic hydrocarbons exhibit an absorption feature at 3.4 micron observed toward sources that sample diffuse regions of the interstellar medium. The absorbers responsible for thi…