127 citations · 357 across the 7 of their papers we have counts for
7 papers
A Tip of the Red Giant Branch Distance of Mpc to the Dark Matter Deficient Galaxy NGC1052-DF2 from 40 Orbits of Hubble Space Telescope Imaging
Zili Shen, Shany Danieli, Pieter van Dokkum +7
The large and diffuse galaxies NGC1052-DF2 and NGC1052-DF4 have been found to have very low dark matter content and a population of luminous globular clusters. Accurate distance me…
When the Peas Jump around the Pod: How Stellar Clustering Affects the Observed Correlations between Planet Properties in Multi-Planet Systems
Mélanie Chevance, J. M. Diederik Kruijssen, Steven N. Longmore
Recent studies have shown that the radii and masses of adjacent planets within a planetary system are correlated. It is unknown how this 'peas-in-a-pod' phenomenon originates, whet…
Applying the Tremaine-Weinberg Method to Nearby Galaxies: Stellar Mass-Based Pattern Speeds, and Comparisons with ISM Kinematics
Thomas G. Williams, Eva Schinnerer, Eric Emsellem +22
We apply the Tremaine-Weinberg method to 19 nearby galaxies using stellar mass surface densities and velocities derived from the PHANGS-MUSE survey, to calculate (primarily bar) pa…
The Physics of Star Cluster Formation and Evolution
Martin G. H. Krause, Stella S. R. Offner, Corinne Charbonnel +8
Star clusters form in dense, hierarchically collapsing gas clouds. Bulk kinetic energy is transformed to turbulence with stars forming from cores fed by filaments. In the most comp…
A model for the minimum mass of bound stellar clusters and its dependence on the galactic environment
Sebastian Trujillo-Gomez, Marta Reina-Campos, J. M. Diederik Kruijssen
We present a simple physical model for the minimum mass of bound stellar clusters as a function of the galactic environment. The model evaluates which parts of a hierarchically-clu…
Star Formation Rates of Massive Molecular Clouds in the Central Molecular Zone
Xing Lu, Qizhou Zhang, Jens Kauffmann +8
We investigate star formation at very early evolutionary phases in five massive clouds in the inner 500 pc of the Galaxy, the Central Molecular Zone. Using interferometer observati…