activity
20242026
collaborators

12 papers

astro-ph.SR2026

Dynamical mass of a solar-like oscillator at the main-sequence turnoff from Gaia astrometry & ground-based spectroscopy

P. G. Beck, T. Masseron, K. Pavlovski +11

Asteroseismology is widely used for precise determining of masses of solar-like oscillating stars by performing individual-frequency modeling or applying homological scaling relati…

astro-ph.IM2025

Spectroscopic Alerts for the Time-Domain Era

Alejandra Melo, Paula Sanchez-Saez, Valentin D. Ivanov +13

Time-domain astronomy is entering an era of unprecedented discovery driven by wide-field, high-cadence surveys such as LSST, Roman, Euclid, SKA, and PLATO. While some of these faci…

astro-ph.IM2025

White Dwarf Binaries: Probes of Future Astrophysics

Anna F. Pala, Roberto Raddi, Alberto Rebassa-Mansergas +25

White dwarf binaries are fundamental astrophysical probes. They represent ideal laboratories to test the models of binary evolution, which also apply to the sources of gravitationa…

astro-ph.SR2025

Identification of new Galactic symbiotic stars with SALT -- II. New discoveries and characterization of the sample

J. Merc, J. Mikołajewska, K. Iłkiewicz +2

We present the continuation of a systematic search for new southern Galactic symbiotic stars, selecting candidates from the SuperCOSMOS H Survey and 2MASS. Follow-up spectrosco…

astro-ph.EP2025

ASASSN-24fw: Candidate circumplanetary disk occultation of a main-sequence star

Nadia L. Zakamska, Gautham Adamane Pallathadka, Dmitry Bizyaev +24

Dusty disks around planetary and substellar companions in outer reaches of exo-planetary systems can be detected as long-lasting occultations, provided the observer is close to the…

astro-ph.SR2025

Revisiting symbiotic binaries with interferometry: II. New PIONIER data

Henri M. J. Boffin, Jaroslav Merc

Symbiotic stars, which generally comprise a red giant and an accreting white dwarf, are excellent laboratories to understand mass transfer in wide binaries, with application to a w…