activity
20192026
collaborators

6 papers

astro-ph.SR2026

Spectroscopic follow-up of Gaia alerted Young Stellar Object variables: the Large Binocular Telescope view

Teresa Giannini, Manuele Gangi, Fernando Cruz-Saenz de Miera +13

We analyzed optical/near-IR Large Binocular Telescope spectra of 16 sources alerted by Gaia between 2021 and 2024 due to significant photometric variability. Half of the spectra we…

astro-ph.SR2025

The 2023 outburst of the Gaia alerted EXor Gaia23bab

Zsófia Nagy, Ágnes Kóspál, Péter Ábrahám +33

Episodic accretion is a fundamental process in the build-up of the stellar mass. EX Lupi-type eruptive young stars (EXors) represent one of the main types of episodic accretion. We…

astro-ph.EP2025

A Multi-Wavelength Study of the Dynamic Environment surrounding the FUor V960 Mon

Philipp Weber, Silvio Ulloa, Sebastián Pérez +11

The evolution of young stars and planet-forming environments is intrinsically linked to their nascent surroundings. This is particularly evident for FU Orionis (FUor) objectsa c…

astro-ph.SR2025

Evidence for an accretion bridge in the DX Cha circumbinary system from VLTI/MATISSE observations

Tímea Juhász, József Varga, Péter Ábrahám +20

DX Cha (HD 104237) is a spectroscopic binary consisting of a Herbig A7.5Ve-A8Ve primary star and a K3-type companion. Here we report on new micrometer interferometric observ…

astro-ph.SR2020

Envelope-to-disk mass transport in the FUor-type young eruptive star V346 Normae

Á. Kóspál, P. Ábrahám, O. Fehér +2

Having disk-to-star accretion rates on the order of 10/yr, FU Orionis-type stars (FUors) are thought to be the visible examples for episodic accretion. FUors are…

astro-ph.SR2019

Resolved ALMA continuum image of the circumbinary ring and circumstellar disks in the L1551 IRS 5 system

Fernando Cruz-Sáenz de Miera, Ágnes Kóspál, Péter Ábrahám +2

L1551 IRS 5 is a FUor-like object located in the Taurus star forming region. We present ALMA 1.3 mm continuum observations using a wide range of baselines. The observations recover…