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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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 observations of SiO masers obtained with the VLA and the VLBA to map the structure and dynamical/temporal evolution of the material 10-1000 AU from the nearest high-mass YSO: Radio Source I in the Orion BN/KL region.
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Trigonometric Parallaxes of Four Star-forming Regions in the Distant Inner Galaxy
Y. Xu,S. B. Bian,Mark J. Reid,J. J. Li,Karl M. Menten,Thomas M. Dame,Bing Zhang,Andreas Brunthaler,Yuefang Wu,Luca Moscadelli,G. Wu,Xingwu Zheng +11 more
TL;DR: This paper measured trigonometric parallaxes for four water masers associated with distant massive young stars in the inner regions of the Galaxy using the VLBA as part of the BeSSeL Survey.
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The structure of the accretion disk in NGC 4258 derived from observations of its water vapor masers
TL;DR: In this paper, the authors obtained a wealth of new information about the structure of the maser disk in NGC 4258 from a series of 18 VLBA observations spanning three years, as well as from 32 epochs of spectral monitoring data from 1994 to the present, acquired with the VLA, Effelsberg, and GBT.
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Methanol and water masers in IRAS 20126+4104: The distance, the disk, and the jet
TL;DR: In this paper, the authors used the Very Long Baseline Array and the European VLBI Network to observe the 22.2 GHz water and 6.7 GHz methanol masers in IRAS 20126+4104 at a number of epochs.
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New Measurements of the Radio Photosphere of Mira based on Data from the JVLA and ALMA
TL;DR: In this paper, the authors measured the millimeter wavelength continuum emission from the long period variable Mira at frequencies of 46 GHz, 96 GHz, and 229 GHz with observations obtained with the Jansky Very Large Array (JVLA) and the Atacama Large Millimeter/submillimeter Array (ALMA).