activity
20242026
collaborators

5 papers

astro-ph.SR2026

KL Dra as a Benchmark Laboratory for Accretion-Disk Physics: Constraints from TESS and Ground-Based Surveys

Luis E. Salazar Manzano, Liliana E. Rivera Sandoval, Jean-Marie Hameury +4

We present the longest-term optical analysis of the AM CVn system KL Dra using years of monitoring from TESS and wide-field ground-based surveys. The continuous TESS cover…

astro-ph.SR2026

A study of transients from ground-based surveys reveals new ultra-compact accreting white dwarf binaries

Jan Kára, Liliana Rivera Sandoval, Wendy Mendoza +5

AM CVn stars are ultra-compact semi-detached binaries consisting of a white dwarf primary and a hydrogen-depleted secondary. In this paper we present spectroscopic and photometric…

astro-ph.HE2025

Massive Double White Dwarf Binary Mergers from the Moon: Extending the Reach of Multi-messenger Astrophysics

Manuel Pichardo Marcano, Anjali B. Yelikar, Karan Jani

We explore the potential of lunar-based gravitational-wave detectors to broaden the multi-messenger astrophysics landscape by detecting mergers of massive () do…

astro-ph.SR2024

A second candidate magnetic helium core white dwarf and 3 other variable white dwarfs in the globular cluster NGC 6397

Manuel Pichardo Marcano, Liliana E. Rivera Sandoval, Thomas J. Maccarone +5

Using archival Hubble Space Telescope observations, we report the discovery of four variable low-mass white dwarfs () in the globular clu…

astro-ph.SR2024

The Temperature versus Orbital Period relation of AM CVns: Insights from their Donors

Colin W. Macrie, Liliana Rivera Sandoval, Yuri Cavecchi +2

We studied the spectral energy distribution (SED) of 22 known AM~CVns with orbital periods () larger than 35~min using multiwavelength public photometric data to estimate…