activity
20022008
most citedIs the SMC Bound to the LMC? The HST Proper Motion of the SMC

275 citations · 676 across the 9 of their papers we have counts for

collaborators

20 papers

astro-ph200830 cited

Caught in formation: the nuclear-cluster-to-be in NGC 2139

David R. Andersen, C. Jakob Walcher, Torsten Boeker +4

Close to its center, the bulgeless galaxy NGC 2139 hosts a star cluster that is younger and less massive than any actual nuclear star cluster (NC) studied so far. We have measured…

astro-ph200851 cited

A New Hubble Space Telescope Distance to NGC 1569: Starburst Properties and IC 342 Group Membership

Aaron J. Grocholski, Alessandra Aloisi, Roeland P. van der Marel +8

We present deep HST ACS/WFC photometry of the dwarf irregular galaxy NGC 1569, one of the closest and strongest nearby starburst galaxies. These data allow us, for the first time,…

astro-ph200736 cited

Constraining the Mass Profiles of Stellar Systems: Schwarzschild Modeling of Discrete Velocity Datasets

Julio Chanamé, Jan Kleyna, Roeland van der Marel

(ABRIDGED) We present a new Schwarzschild orbit-superposition code designed to model discrete datasets composed of velocities of individual kinematic tracers in a dynamical system.…

astro-ph2007125 cited

M31 Transverse Velocity and Local Group Mass from Satellite Kinematics

Roeland P. van der Marel, Puragra Guhathakurta

We present several different statistical methods to determine the transverse velocity vector of M31. The underlying assumptions are that the M31 satellites on average follow the mo…

astro-ph200724 cited

The Toomre Sequence Revisited with HST/NICMOS: Nuclear Brightness Profiles and Colors of Interacting and Merging Galaxies

Joern Rossa, Seppo Laine, Roeland P. van der Marel +4

We discuss the near-infrared properties of the nuclei in the 11 merging galaxies of the Toomre sequence, based on high spatial resolution J, H, and K imaging data using NICMOS onbo…

astro-ph200652 cited

Dynamical Models of Elliptical Galaxies in z=0.5 Clusters: II. Mass-to-Light Ratio Evolution without Fundamental Plane Assumptions

Roeland P. van der Marel, Pieter G. van Dokkum

We study M/L evolution of early-type galaxies using dynamical modeling of resolved internal kinematics. This makes fewer assumptions than Fundamental Plane (FP) studies and provide…