activity
20092026
most citedThe Red MSX Source Survey: the Massive Young Stellar Population of our Galaxy

289 citations · 2.6k across the 34 of their papers we have counts for

collaborators

34 papers

astro-ph.SR2026

A survey for variable young stars with small telescopes - XI. Spot Lifetimes and Coverage Distributions

Dirk Froebrich, Carys Herbert, Aleks Scholz +47

We present a homogeneous analysis of rotational variability and spot properties in young stellar objects across multiple star-forming regions observed by the Hunting Outbursting Yo…

astro-ph.SR2024

A survey for variable stars with small telescopes: IX -- Evolution of Spot Properties on YSOs in IC5070

Carys Herbert, Dirk Froebrich, Siegfried Vanaverbeke +45

We present spot properties on 32 periodic young stellar objects in IC 5070. Long term, 5 yr, light curves in the , , and -bands are obtained through the HOYS (Huntin…

astro-ph.GA2020★ 16 cited

ATLASGAL -- Relationship between dense star forming clumps and interstellar masers

S. J. Billington, J. S. Urquhart, C. König +10

We have used catalogues from several Galactic plane surveys and dedicated observations to investigate the relationship between various maser species and Galactic star forming clump…

astro-ph.SR2019★ 21 cited

Fragmentation, rotation and outflows in the high-mass star-forming region IRAS 23033+5951. A case study of the IRAM NOEMA large program CORE

F. Bosco, H. Beuther, A. Ahmadi +23

The formation process of high-mass stars (>8M) is poorly constrained, particularly, the effects of clump fragmentation creating multiple systems and the mechanism of mass a…

astro-ph.SR2018★ 9 cited

Extreme star formation in the Milky Way: Luminosity distributions of young stellar objects in W49A and W51

D. J. Eden, T. J. T. Moore, J. S. Urquhart +8

We have compared the star-formation properties of the W49A and W51 regions by using far-infrared data from the Herschel infrared Galactic Plane Survey (Hi-GAL) and 850-um observati…

astro-ph.GA2017★ 33 cited

The evolution of young HII regions

P. D. Klaassen, K. G. Johnston, J. S. Urquhart +6

High-mass stars form in much richer environments than those associated with isolated low-mass stars, and once they reach a certain mass, produce ionised (HII) regions. The formatio…

astro-ph.GA2017★ 43 cited

H2O Southern Galactic Plane Survey (HOPS): Paper III - Properties of Dense Molecular Gas across the Inner Milky Way

S. N. Longmore, A. J. Walsh, C. R. Purcell +22

The H2O Southern Galactic Plane Survey (HOPS) has mapped 100 square degrees of the Galactic plane for water masers and thermal molecular line emission using the 22-m Mopra telescop…

astro-ph.GA2016★ 101 cited

A search for ionized jets towards massive young stellar objects

S. J. D. Purser, S. L. Lumsden, M. G. Hoare +7

Radio continuum observations using the Australia telescope compact array at 5.5, 9.0, 17.0 and 22.8 GHz have detected free-free emission associated with 45 of 49 massive young stel…

astro-ph.SR2015★ 110 cited

Infall through the evolution of high-mass star-forming clumps

F. Wyrowski, R. Güsten, K. M. Menten +6

With the GREAT receiver at the Stratospheric Observatory for Infrared Astronomy (SOFIA), nine massive molecular clumps have been observed in the ammonia line at 1.…

astro-ph.SR2015★ 41 cited

A distance limited sample of massive star forming cores from the RMS survey

L. T. Maud, S. L. Lumsden, T. J. T. Moore +3

We analyse CO (2) data from a sample of 99 infrared-bright massive young stellar objects (MYSOs) and compact HII regions that were identified as potential molecular-ou…

astro-ph.GA2015★ 16 cited

Infrared dark clouds on the far side of the Galaxy

A. Giannetti, F. Wyrowski, S. Leurini +5

Context: Infrared dark clouds are the coldest and densest portions of giant molecular clouds. The most massive ones represent some of the most likely birthplaces for the next gener…

astro-ph.SR2015★ 28 cited

6.7GHz Methanol Maser Associated Outflows: An evolutionary sequence

H. M. de Villiers, A. Chrysostomou, M. A. Thompson +8

We present a continuing study of a sample 44 molecular outflows, observed in 13CO lines, closely associated with 6.7GHz methanol masers, hence called Methanol Maser Associated Outf…

astro-ph.SR2014★ 54 cited

Methanol Maser Associated Outflows: Detection statistics and properties

H. M. de Villiers, A. Chrysostomou, M. A. Thompson +6

We have selected the positions of 54 6.7GHz methanol masers from the Methanol Multibeam Survey catalogue, covering a range of longitudes between and of th…

astro-ph.GA2014★ 108 cited

ATLASGAL --- Complete compact source catalogue: 280\degr\ 60\degr

J. S. Urquhart, T. Csengeri, F. Wyrowski +9

The APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) is the largest and most sensitive systematic survey of the inner Galactic plane in the submillimetre wavelength regime…

astro-ph.GA2014★ 241 cited

ATLASGAL --- towards a complete sample of massive star forming clumps

J. S. Urquhart, T. J. T. Moore, T. Csengeri +12

By matching infrared-selected, massive young stellar objects (MYSOs) and compact HII regions in the RMS survey to massive clumps found in the submillimetre ATLASGAL survey, we have…

astro-ph.GA2014★ 8 cited

Molecular line mapping of the giant molecular cloud associated with RCW 106 - IV. Ammonia towards dust emission

Vicki Lowe, Maria R. Cunningham, James S. Urquhart +6

Here we report observations of the two lowest inversion transitions of ammonia with the 70-m Tidbinbilla radio telescope. They were conducted to determine the kinetic temperatures…

astro-ph.GA2013★ 171 cited

The RMS Survey: Galactic distribution of massive star formation

J. S. Urquhart, C. C. Figura, T. J. T. +6

Abridged: We have used the well-selected sample of ~1750 embedded, young, massive stars identified by the RMS survey to investigate the Galactic distribution of recent massive star…

astro-ph.GA2013★ 289 cited

The Red MSX Source Survey: the Massive Young Stellar Population of our Galaxy

S. L. Lumsden, M. G. Hoare, J. S. Urquhart +5

We present the Red MSX Source (RMS) Survey, the largest statistically selected catalog of young massive protostars and HII regions to date. We outline the construction of the catal…

astro-ph.GA2013★ 155 cited

ATLASGAL --- properties of compact HII regions and their natal clumps

J. S. Urquhart, M. A. Thompson, T. J. T. Moore +13

We present a complete sample of molecular clumps containing compact and ultra-compact (UC) HII regions between \ell=10\degr and 60\degr\ and $|b|<1\degr, identified by combining th…

astro-ph.IM2013★ 56 cited

Characterization of the MALT90 Survey and the Mopra Telescope at 90 GHz

Jonathan B. Foster, Jill M. Rathborne, Patricio Sanhueza +23

We characterize the Millimeter Astronomy Legacy Team 90 GHz (MALT90) Survey and the Mopra telescope at 90 GHz. We combine repeated position-switched observations of the source G300…

astro-ph.GA2013★ 93 cited

Star formation in Galactic spiral arms and the inter-arm regions

D. J. Eden, T. J. T. Moore, L. K. Morgan +2

The line of sight through the Galactic Plane between longitudes l = 37.83 degr and l = 42.50 degr allows for the separation of Galactic Ring Survey molecular clouds into those that…

astro-ph.GA2013★ 168 cited

ATLASGAL --- Environments of 6.7\,GHz methanol masers

J. S. Urquhart, T. J. T. Moore, F. Schuller +7

Using the 870-m APEX Telescope Large Area Survey of the Galaxy (ATLASGAL), we have identified 577 submillimetre continuum sources with masers from the methanol multibeam (MMB) s…

astro-ph.GA2013★ 94 cited

The RMS Survey: Near-IR Spectroscopy of Massive Young Stellar Objects

H. D. B. Cooper, S. L. Lumsden, R. D. Oudmaijer +6

Near-infrared H- and K-band spectra are presented for 247 objects, selected from the Red MSX Source (RMS) survey as potential young stellar objects (YSOs). 195 (~80%) of the target…

astro-ph.GA2012★ 34 cited

The G305 star-forming complex: Embedded Massive Star Formation Discovered by Herschel Hi-GAL

A. Faimali, M. A. Thompson, L. Hindson +7

We present a Herschel far-infrared study towards the rich massive star- forming complex G305, utilising PACS 70, 160 μm and SPIRE 250, 350, and 500 μm observations from the Hi-GAL…