Repeating Outbursts from the Young Stellar Object Gaia23bab (= SPICY 97589)
| Autor: | Michael A. Kuhn, Robert A. Benjamin, Emille E. O. Ishida, Rafael S. de Souza, Julien Peloton, Michele Delli Veneri |
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| Přispěvatelé: | Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS) |
| Jazyk: | angličtina |
| Rok vydání: | 2023 |
| Předmět: | |
| Zdroj: | Res.Notes AAS Res.Notes AAS, 2023, 7 (3), pp.57. ⟨10.3847/2515-5172/acc4c9⟩ |
| DOI: | 10.3847/2515-5172/acc4c9⟩ |
| Popis: | The light curve of Gaia23bab (= SPICY 97589) shows two significant ($ΔG>2$ mag) brightening events, one in 2017 and an ongoing event starting in 2022. The source's quiescent spectral energy distribution indicates an embedded ($A_V>5$ mag) pre-main-sequence star, with optical accretion emission and mid-infrared disk emission. This characterization is supported by the source's membership in an embedded cluster in the star-forming cloud DOBASHI 1604 at a distance of $900\pm45$~pc. Thus, the brightening events are probable accretion outbursts, likely of EX Lup-type. 4 pages and 1 figure. Submitted to Research Notes of the AAS |
| Databáze: | OpenAIRE |
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