M
Mark J. Reid
Researcher at Smithsonian Institution
Publications - 466
Citations - 33032
Mark J. Reid is an academic researcher from Smithsonian Institution. The author has contributed to research in topics: Galaxy & Maser. The author has an hindex of 89, co-authored 456 publications receiving 30293 citations. Previous affiliations of Mark J. Reid include Max Planck Society & California Institute of Technology.
Papers
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Book ChapterDOI
Proper motion studies of H2O masers
TL;DR: The work of the CfA group over the past decade to measure the proper motions of H2O masers in our Galaxy is described in this article, where distances to 7 masers have been measured and the distance to the Galactic Center, Ro, is estimated to be 7.6 ± 0.6 kpc.
Journal ArticleDOI
Erratum - the Structure of OH Masers around Late-Type Stars
Book ChapterDOI
Proper Motions in the Andromeda Subgroup
TL;DR: In this paper, VLBI observations of regions of H2O maser activity in the Local Group galaxies M33 and IC10 were used to measure the proper motions of the two galaxies.
Posted Content
Maser Astrometry with VLBI and the SKA
James Green,Huib Jan van Langevelde,Andreas Brunthaler,Simon Ellingsen,Hiroshi Imai,Wouter Vlemmings,Mark J. Reid,Anita M. S. Richards +7 more
TL;DR: The Square Kilometre Array (SKA) as mentioned in this paper has been proposed to provide trigonometric distances with errors as small as 1% for the first phase of the SKA, which will enable observations of hydroxyl and methanol masers to an accuracy of 5 microarcseconds.
Journal ArticleDOI
A documentary of high-mass star formation: Probing the dynamical evolution of Orion Source I on 10–100 AU scales using SiO masers
Lynn D. Matthews,Ciriaco Goddi,L. J. Greenhill,Claire J. Chandler,Mark J. Reid,Elizabeth Humphreys +5 more
TL;DR: The KaLYPSO project as discussed by the authors uses SiO masers obtained with the Very Large Array (VLA) and the Very Long Baseline Array (VLBA) to map the structure and dynamical/temporal evolution of the material 10-1000 AU from the nearest high-mass radio source I in the Orion BN/KL region.