J
James Schombert
Researcher at University of Oregon
Publications - 108
Citations - 6390
James Schombert is an academic researcher from University of Oregon. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 36, co-authored 101 publications receiving 5386 citations. Previous affiliations of James Schombert include California Institute of Technology & University of Michigan.
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Journal ArticleDOI
The Baryonic Tully-Fisher Relation.
TL;DR: In this paper, the authors explore the Tully-Fisher relation over five decades in stellar mass in galaxies with circular velocities ranging over 30 Vc 300 km s-1.
Journal ArticleDOI
Radial Acceleration Relation in Rotationally Supported Galaxies.
TL;DR: A correlation between the radial acceleration traced by rotation curves and that predicted by the observed distribution of baryons is reported, tantamount to a natural law for rotating galaxies.
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Sparc: mass models for 175 disk galaxies with spitzer photometry and accurate rotation curves
TL;DR: SPARC (Spitzer Photometry & Accurate Rotation Curves) as mentioned in this paper is a sample of 175 nearby galaxies with new surface photometry at 3.6 um and high-quality rotation curves from previous HI/Halpha studies.
Journal ArticleDOI
One Law To Rule Them All: The Radial Acceleration Relation of Galaxies
Federico Lelli,Federico Lelli,Stacy S. McGaugh,James Schombert,Marcel S. Pawlowski,Marcel S. Pawlowski +5 more
TL;DR: In this paper, the authors studied the radial acceleration relation between baryons and dark matter in 240 galaxies with spatially resolved kinematic data and found that the relationship coincides with the 1:1 line (no dark matter) at high accelerations but systematically deviates from unity below a critical scale of ~10^-10 m/s^2.
Journal ArticleDOI
SPARC: Mass Models for 175 Disk Galaxies with Spitzer Photometry and Accurate Rotation Curves
TL;DR: SPARC (Spitzer Photometry & Accurate Rotation Curves) as mentioned in this paper is a sample of 175 nearby galaxies with new surface photometry at 3.6 um and high-quality rotation curves from previous HI/Halpha studies.