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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Proceedings ArticleDOI
A preliminary distance to W75N in the Cygnus X star-forming region
Andreas Brunthaler,Kazi L.J. Rygl,Karl M. Menten,Mark J. Reid,Huib Jan van Langevelde,Mareki Honma,K. Torstensson,Kenta Fujisawa,Alberto Sanna +8 more
TL;DR: Rygl et al. as mentioned in this paper proposed a method to detect the presence of the Earth's magnetic field at the Max-Planck-Institut fur Radioastronomie (MPIfR).
Journal ArticleDOI
The Intrinsic Shape of Sagittarius A* at 3.5-mm Wavelength
Gisela N. Ortiz-León,Michael D. Johnson,Sheperd S. Doeleman,Sheperd S. Doeleman,Lindy Blackburn,Vincent L. Fish,Laurent Loinard,Laurent Loinard,Mark J. Reid,Edgar Castillo,Andrew A. Chael,Antonio Hernández-Gómez,David H. Hughes,Jonathan León-Tavares,Jonathan León-Tavares,Ru-Sen Lu,Alfredo Montaña,Gopal Narayanan,Katherine A. Rosenfeld,David Sánchez,F. Peter Schloerb,Zhi-Qiang Shen,Hotaka Shiokawa,Jason SooHoo,Laura Vertatschitsch +24 more
TL;DR: In this paper, the authors used the known scattering kernel to determine the intrinsic two-dimensional source size at 3.5 mm: $(147\pm7~\mu\rm{as})
Posted Content
Science with an ngVLA: A six-dimensional tomographic view of Galactic star-formation
Laurent Loinard,Mark J. Reid +1 more
TL;DR: In this paper, the authors proposed a very long baseline interferometry (VLBI) radio array with baselines extending to several thousand km to provide a full six-dimensional view (three spatial and three velocity coordinates) of star formation in the Galactic disk.
Journal ArticleDOI
Astrometry and proper motions with space VLBI
TL;DR: In this paper, the use of space VLBI for the measurement of proper motions of extragalactic H2O masers is discussed, even with baseline accuracies significantly less accurate than achievable on the ground.
Book ChapterDOI
Shocks in the Radio Photospheres of Long Period Variable Stars
Mark J. Reid,Karl M. Menten +1 more
TL;DR: In this article, Danchi et al. studied the region between the optical photosphere and the dust formation zone in a Mira variable and found that a significant fraction of the mass returned to the interstellar medium comes from red giant stars.