M
Marc Verheijen
Researcher at Kapteyn Astronomical Institute
Publications - 209
Citations - 11216
Marc Verheijen is an academic researcher from Kapteyn Astronomical Institute. The author has contributed to research in topics: Galaxy & Galaxy cluster. The author has an hindex of 53, co-authored 202 publications receiving 10327 citations. Previous affiliations of Marc Verheijen include University of Wisconsin-Madison & University of Groningen.
Papers
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(intrinsic) Variations of Wolf-Rayet Stars
A. M. van Genderen,Marc Verheijen,K. A. van der Hucht,C. De Loore,H. E. Schwarz,B. P. M. van Esch,H. Greidanus,R. van der Heiden,E. van Kampen,E. Kuulkers,R. S. Le Poole,R. A. Reijns,F. H. A. Robijn,L. Spijkstra +13 more
The Stability of Galaxy Disks
Kyle B. Westfall,David R. Andersen,Matthew A. Bershady,Thomas P. K. Martinsson,R. A. Swaters,Marc Verheijen +5 more
TL;DR: In this paper, the stellar surface mass density (Σ*) and two-component (gas+stars) disk stability (QRW) for 25 late-type galaxies from the DiskMass Survey were calculated using a Markov Chain Monte Carlo sampling of the Bayesian posterior.
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CO mapping of spiral galaxies in the Ursa Major cluster: An atlas
TL;DR: The first results of the On-The-Fly (OTF) CO(J=1-0) mapping of spiral galaxies in the Ursa Major cluster were obtained with the NRAO 12m radio telescope during June 20-27-1999 and March 23-30, 2000 as mentioned in this paper.
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An HI Study of Ursa Major Spirals
TL;DR: In this paper, the authors investigate the scatter in the TF-relations and study the Dark Matter component of spiral galaxies as a function of luminosity, morphology, scale length etc by means of a detailed kinematic and photometric study of individual galaxies in a cluster.
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Mass distributions in disk galaxies
T. Martinsson,Marc Verheijen,Matthew A. Bershady,Kyle B. Westfall,David R. Andersen,R. A. Swaters +5 more
TL;DR: In this paper, the authors present results on luminous and dark matter distributions in disk galaxies from the DiskMass Survey, finding that stars dominate the baryonic mass budget in the inner region of the disk; however, at about four optical scale lengths (hR ) the atomic gas starts to become the dominant contributor.