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

289 citations · 3.4k across the 70 of their papers we have counts for

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Showing 2009Show all

6 papers · 1 filter

astro-ph.GA2009★ 30 cited

The RMS Survey: Far-Infrared Photometry of Young Massive Stars

J. C. Mottram, M. G. Hoare, S. L. Lumsden +5

Context: The Red MSX Source (RMS) survey is a multi-wavelength campaign of follow-up observations of a colour-selected sample of candidate massive young stellar objects (MYSOs) in…

astro-ph.SR2009★ 55 cited

The origin of mid-infrared emission in massive young stellar objects: multi-baseline VLTI observations of W33A

W. J. de Wit, M. G. Hoare, R. D. Oudmaijer +1

The circumstellar structure on 100 AU scales of the massive young stellar object W33A is probed using the VLTI and the MIDI instrument. N-band visibilities on 4 baselines are prese…

astro-ph.SR2009★ 74 cited

The mass ratio and formation mechanisms of Herbig Ae/Be star binary systems

H. E. Wheelwright, R. D. Oudmaijer, S. P. Goodwin

We present B and R band spectroastrometry of a sample of 45 Herbig Ae/Be stars in order to study their binary properties. All but one of the targets known to be binary systems with…

astro-ph.SR2009★ 44 cited

On the presence and absence of disks around O-type stars

Jorick S. Vink, B. Davies, T. J. Harries +2

(abridged) As the favoured progenitors of long-duration gamma-ray bursts, massive stars may represent our best signposts of individual objects in the early Universe, but special co…

astro-ph.GA2009★ 174 cited

The RMS Survey: 6 cm continuum VLA observations towards candidate massive YSOs in the northern hemisphere

J. S. Urquhart, M. G. Hoare, C. R. Purcell +6

(Abridged) Context: The Red MSX Source (RMS) survey is an ongoing multi-wavelength observational programme designed to return a large, well-selected sample of massive young stellar…

astro-ph.SR2009★ 9 cited

The close Be star companion of Beta Cephei

H. E. Wheelwright, R. D. Oudmaijer, R. S. Schnerr

The prototype of the Beta Cep class of pulsating stars, Beta Cep, rotates relatively slowly, and yet displays episodic Halpha emission. Such behaviour is typical of a classical Be…