The Gaia alerted fading of the FUor-type star Gaia21elv
Zs\'ofia Nagy, Sunkyung Park, P\'eter \'Abrah\'am, \'Agnes K\'osp\'al,, Fernando Cruz-S\'aenz de Miera, M\'aria Kun, Micha{\l} Siwak, Zs\'ofia, Marianna Szab\'o, M\'at\'e Szil\'agyi, Eleonora Fiorellino, Teresa Giannini,, Jae-Joon Lee, Jeong-Eun Lee, G\'abor Marton

TL;DR
This study documents the fading of Gaia21elv, a FUor-type young star, through multi-epoch spectroscopy and photometry, revealing typical FUor features and a likely increase in circumstellar extinction during its decline.
Contribution
It provides detailed spectroscopic and photometric analysis of Gaia21elv's fading, confirming it as a classical FUor and identifying signs of jet activity and changing accretion rates.
Findings
Gaia21elv shows typical FUor spectral signatures.
Fading is likely due to increased circumstellar extinction.
Spectral analysis indicates a decrease in accretion rate.
Abstract
FU Orionis objects (FUors) are eruptive young stars, which exhibit outbursts that last from decades to a century. Due to the duration of their outbursts, and to the fact that only about two dozens of such sources are known, information on the end of their outbursts is limited. Here we analyse follow-up photometry and spectroscopy of Gaia21elv, a young stellar object, which had a several decades long outburst. It was reported as a Gaia science alert due to its recent fading by more than a magnitude. To study the fading of the source and look for signatures characteristic of FUors, we have obtained follow-up near infrared (NIR) spectra using Gemini South/IGRINS, and both optical and NIR spectra using VLT/X-SHOOTER. The spectra at both epochs show typical FUor signatures, such as a triangular shaped -band continuum, absorption-line dominated spectrum, and P Cygni profiles. In addition…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Astro and Planetary Science · Space Exploration and Technology
