Historically, FU Orionis-type stars are low-mass, pre-main-sequence stars. The members of this class experience powerful accretion outbursts and remain in an...
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PublicationA Multi-epoch, Multiwavelength Study of the Classical FUor V1515 Cyg Approaching Quiescence
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PublicationA Study of the Photometric and Spectroscopic Variations of the Prototypical FU Orionis-type Star V1057 Cyg
Among the low-mass pre-main sequence stars, a small group called FU Orionis-type objects (FUors) are notable for undergoing powerful accretion outbursts. V1057...
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PublicationAssessing the Stellar Population and the Environment of an H II Region on the Far Side of the Galaxy
We have investigated the stellar and interstellar content of the distant star formation region IRAS 17591-2228 (WISE H II region GAL 007.47+0.06). It is...
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PublicationRecurrent Strong Outbursts of an EXor-like Young Eruptive Star Gaia20eae
We present follow-up photometric and spectroscopic observations, and subsequent analysis of Gaia20eae. This source triggered photometric alerts during 2020...
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PublicationTOI-4562b: A Highly Eccentric Temperate Jupiter Analog Orbiting a Young Field Star
We report the discovery of TOI-4562b (TIC-349576261), a Jovian planet orbiting a young F7V-type star, younger than the Praesepe/Hyades clusters (<700 Myr). This...
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PublicationUnderstanding the Angular Momentum Evolution of T Tauri and Herbig Ae/Be Stars
We investigate a sample of six Herbig Ae/Be stars belonging to the Orion OB1 association, as well as 73 low-mass objects, members of the σ Orionis cluster, in...