activity
20242026
collaborators

21 papers

astro-ph.GA2026

A Long Period Stellar-Mass Black Hole Binary in Centauri

Matthew Whitaker, Evan Kerr, Anil Seth +16

Modern simulations of stellar dynamics in globular clusters peg a dominant role for stellar-mass black holes, but direct evidence for black holes in clusters remains limited. We pr…

astro-ph.SR2026

Stellar rotation and binaries in open clusters with Gaia DR3

Elena Pancino, Elisabetta Reggiani, Silvia Marinoni +14

Stellar rotation is a fundamental ingredient in shaping the evolution of stars and it can also be used to trace past stellar interactions. Yet, systematic studies of stellar rotati…

astro-ph.GA2026

The MUSE-Faint survey V. The binary fraction of Leo T

Daniel Vaz, Jarle Brinchmann, Sebastian Kamann +3

The Leo T dwarf galaxy, the faintest and least massive galaxy known to have recent star formation (), exhibits a high dynamical mass-to-light ratio based on its stellar…

astro-ph.GA2026

oMEGACat. IX. Chemical Tagging of Omega Centauri Populations with Machine-Learning-Inferred Abundances from the MUSE Spectrograph

Z. Wang, A. C. Seth, C. Clontz +14

We present chemical abundance measurements for 7,302 red giant branch stars within the half-light radius (~5') of Centauri ( Cen), derived from MUSE spectra using the neur…

astro-ph.SR2026

Discovery of a double white dwarf in the Galactic globular cluster NGC 6397

Fabian Göttgens, Marilyn Latour, Ulrich Heber +4

Binaries in the cores of globular clusters are known to prevent the gravitational collapse of the cluster, and simulations predict that the core of NGC 6397 contains a large number…

astro-ph.IM2026

The SPace-based InterFerometer Feasibility (SPIFF) Project: Enabling Future High-Resolution Astronomy Across the EM Spectrum

Berke Vow Ricketti, Victoria Yankelevich, Chris Benson +19

A plethora of astronomical science cases can only be achieved with high angular resolution observations, and we can expect the number of these to grow as astronomers are constraine…