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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Journal ArticleDOI
Subarcsecond Submillimeter Continuum Observations of Orion KL
Henrik Beuther,Qizhou Zhang,Lincoln J. Greenhill,Mark J. Reid,David J. Wilner,Eric Keto,Daniel P. Marrone,Paul T. P. Ho,James M. Moran,Ramprasad Rao,H. Shinnaga,Sheng-Yuan Liu +11 more
TL;DR: In this paper, the first 865 μm image with sub-arcsecond resolution obtained with the Submillimeter Array was presented, which resolved the Orion KL region into the hot core, the nearby radio source I, the sub-millimeter counterpart to the infrared source n (radio source L), and new submillimeter continuum sources.
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The Distance, Inclination, and Spin of the Black Hole Microquasar H1743-322
TL;DR: In this paper, a simple and symmetric kinematic model was applied to the trajectories of two-sided radio and X-ray jets of H1743-322 to determine the source distance, 8.5 \pm 0.8 kpc and inclination angle of the jets, 75 \pm 3 degrees.
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The local spiral structure of the Milky Way.
Ye Xu,Mark J. Reid,Thomas M. Dame,Karl M. Menten,Nobuyuki Sakai,J. J. Li,Andreas Brunthaler,Luca Moscadelli,Bo Zhang,X. W. Zheng +9 more
TL;DR: Observed regions of massive star formation near the Local spiral arm of the Milky Way reveal that the Local Arm is larger than previously thought, and both its pitch angle and star formation rate are comparable to those of the Galaxy’s major spiral arms, such as Sagittarius and Perseus.
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DISTANCE AND KINEMATICS OF THE RED HYPERGIANT VY CMa: VERY LONG BASELINE ARRAY AND VERY LARGE ARRAY ASTROMETRY
TL;DR: In this paper, the authors measured a trigonometric parallax of 0.53 to be alpha(J2000) = 07(h)22(m)58.(s)3259 +/- 0.0007, delta(J 2000) =-25 degrees 46'03''063 +/- 0.''010.
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II. Accurate Positions and Proper Motions of Stellar SiO Masers near the Galactic Center
TL;DR: In this article, the authors reported greatly improved radio positions and proper motions of many stellar SiO masers at the Galactic Center, and the central stellar cluster moves with Sgr A* to within approximatly 70 km/s.