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Pengfei Li

4 papers hereh-index 12640 citations35 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author1
  • last author3

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
same name
  • Pengfei Li — 12 papers, h 2
  • Pengfei Li — 11 papers, h 4
  • Pengfei Li — 10 papers, h 14
  • Pengfei Li — 8 papers, h 3
  • Pengfei Li — 7 papers, h 11
  • Pengfei Li — 7 papers, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators

4 papers

astro-ph.GA2024

The empirical laws of galaxy dynamics: from gas kinematics to weak lensing

Federico Lelli, Tobias Mistele, Stacy S. McGaugh +2

Galaxies obey a set of strict dynamical laws, which imply a close coupling between the visible matter (stars and gas) and the observed dynamics (set by dark matter in the standard…

astro-ph.GA2024

Indefinitely Flat Circular Velocities and the Baryonic Tully-Fisher Relation from Weak Lensing

Tobias Mistele, Stacy McGaugh, Federico Lelli +2

We use a new deprojection formula to infer the gravitational potential around isolated galaxies from weak gravitational lensing. The results imply circular velocity curves that rem…

astro-ph.GA2024

Radial acceleration relation of galaxies with joint kinematic and weak-lensing data

Tobias Mistele, Stacy McGaugh, Federico Lelli +2

We combine kinematic and gravitational lensing data to construct the Radial Acceleration Relation (RAR) of galaxies over a large dynamic range. We improve on previous weak-lensing…

astro-ph.GA2024

A Distinct Radial Acceleration Relation across Brightest Cluster Galaxies and Galaxy Clusters

Yong Tian, Chung-Ming Ko, Pengfei Li +2

Recent studies reveal a radial acceleration relation (RAR) in galaxies, which illustrates a tight empirical correlation connecting the observational acceleration and the baryonic a…

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