collaborators

10 papers

astro-ph.GA2026

Beyond traditional emission-line diagnostics: using autoencoders to uncover active galactic nuclei in DESI spectra

J. A. Alcolea, M. Siudek, M. Eriksen +49

The growing volume of spectroscopic data in modern surveys motivates data-driven approaches that complement traditional emission-line diagnostics for active galactic nuclei (AGN) i…

astro-ph.SR2026

Detection of unidentified molecular pure rotational lines in C-rich PNe I. The fullerene-containing PN IC 418

T. Huertas-Roldán, J. P. Fonfría, J. Alcolea +7

Molecular emission is observed in a wide variety of astrophysical environments, yet a substantial fraction of spectral features detected at mm wavelengths remains unidentified. Ide…

astro-ph.SR2026

VLTI/PIONIER imaging of post-AGB binaries. An INSPIRING hunt for inner rim substructures in circumbinary discs

Toon De Prins, Akke Corporaal, Jacques Kluska +10

We image the detailed inner rim morphology for a sample of post-AGB circumbinary discs observed using NIR interferometry. At resolutions down to ~1-2 mas (corresponding to ~1-10 AU…

astro-ph.SR2026

Chemistry in the High expansion-velocity C-rich evolved star AFGL2233. Isotopic ratios, peculiarities and evolutionary status

G. Quintana-Lacaci, M. Agúndez, L. Velilla-Prieto +4

High expansion velocity carbon stars (HVCs) are a rare class of evolved stars whose circumstellar envelopes (CSEs) combine C-rich chemistry with unusually high expansion velocities…

astro-ph.SR2025

CO observations in rotating circumbinary post-AGB disks

I. Gallardo Cava, J. Alcolea, H. Van Winckel +3

There is a group of post-AGB stars that are part of a binary system and that show a significant NIR excess. These systems are known to host disks with Keplerian or quasi-Keplerian…

astro-ph.SR2025

Newborn jet in the symbiotic system R Aquarii

T. Liimets, D. P. K. Banerjee, M. Santander-García +12

R Aquarii (R Aqr) is a well-known symbiotic binary that has attracted renewed interest during its recent periastron passage, an event that occurs only once every about 40 years. Th…