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.
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Book ChapterDOI
The Bar and Spiral Structure Legacy (BeSSeL) Survey: Mapping the Milky Way with VLBI Astrometry†
Andreas Brunthaler,Mark J. Reid,K. M. Menten,Xingwu Zheng,Anna Bartkiewicz,Y. K. Choi,Thomas M. Dame,K. Hachisuka,K. Immer,K. Immer,G. A. Moellenbrock,Luca Moscadelli,K. L. J. Rygl,K. L. J. Rygl,Alberto Sanna,Mayumi Sato,Yuanwei Wu,Ye Xu,B. Zhang +18 more
TL;DR: In this article, the authors present an update on the first results, implementing a recent change in the knowledge about the Solar motion, and give an outlook to future observations in the Bar and Spiral Structure Legacy (BeSSeL) survey.
Journal ArticleDOI
Neutral Hydrogen 21cm Absorption at Redshift 0.673 towards 1504+377
TL;DR: In this article, the authors detect the 21 cm line of neutral hydrogen in absorption at a redshift of 0673 towards the 1 Jy radio source 1504+377, which is located toward the center of what appears to be an inclined disk galaxy at z = 0674 The 21 cm absorption line shows multiple velocity components over a velocity range of about 100 km sec$^{-1}, with a total HI column density: N(HI) = $38\times10^{19}\times({{T_s}\over{f}})$ cm$^{
Journal ArticleDOI
Observations of OH and H 2 O microwave maser emission from VY Canis Majoris.
B. R. Rosen,James M. Moran,Mark J. Reid,R. C. Walker,Bernard F. Burke,K. J. Johnston,J. H. Spencer +6 more
Journal ArticleDOI
On Estimating the Mass of Keplerian Accretion Disks in H2O Maser Galaxies
TL;DR: In this article, a 3D Bayesian model for H2O maser disks was proposed to place better constraints on the disk masses of Keplerian maser systems and also evaluate constraints based on the physical conditions for disks which support water maser emission.