activity
20022009
most citedToward a New Distance to the Active Galaxy NGC 4258: II. Centripetal Accelerations and Investigation of Spiral Structure

88 citations · 251 across the 4 of their papers we have counts for

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astro-ph200788 cited

Toward a New Distance to the Active Galaxy NGC 4258: II. Centripetal Accelerations and Investigation of Spiral Structure

E. M. L. Humphreys, M. J. Reid, L. J. Greenhill +2

We report measurements of centripetal accelerations of maser spectral components of NGC 4258 for 51 epochs spanning 1994 to 2004. This is the second paper of a series, in which the…

astro-ph20073 cited

The structure of the accretion disk in NGC 4258 derived from observations of its water vapor masers

Jim Moran, Liz Humphreys, Lincoln Greenhill +2

A wealth of new information about the structure of the maser disk in NGC 4258 has been obtained from a series of 18 VLBA observations spanning three years, as well as from 32 addit…

astro-ph200779 cited

Imaging the Ionized Disk of the High-Mass Protostar Orion-I

M. J. Reid, K. M. Menten, L. J. Greenhill +1

We have imaged the enigmatic radio source-I (Orion-I) in the Orion-KL nebula with the VLA at 43 GHz with 34 mas angular resolution. The continuum emission is highly elongated and i…

astro-ph2005

The Distance to the Perseus Spiral Arm in the Milky Way

Y. Xu, M. J. Reid, X. W. Zheng +1

We have measured the distance to the massive star-forming region W3OH in the Perseus spiral arm of the Milky Way to be 1.95 0.04 kilo-parsecs ( km). This d…

astro-ph2004

Sub-arcsecond sub-mm continuum observations of Orion-KL

H. Beuther, Q. Zhang, L. J. Greenhill +9

We present the first 865 mu continuum image with sub-arcsecond resolution obtained with the Submillimeter Array. These data resolve the Orion-KL region into the hot core, the nearb…

astro-ph2002

Closest Star Seen Orbiting the Supermassive Black Hole at the Centre of the Milky Way

R. Schodel, T. Ott, R. Genzel +20

Measurements of stellar velocities and variable X-ray emission near the centre of the Milky Way have provided the strongest evidence so far that the dark mass concentrations seen i…