From the 1 of 80 papers with an AI index.
77 citations
- Institute for Fundamental Physics of the UniverseIT57 papers
- National Institute for AstrophysicsIT49 papers
- Aix-Marseille UniversitéFR48 papers
- Brera Astronomical ObservatoryIT48 papers
- Instituto de Astrofísica de CanariasES48 papers
- Astronomical Observatory of RomeIT46 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di TriesteIT46 papers
- Centro de Investigaciones Energéticas, Medioambientales y TecnológicasES45 papers
- Institute of Space SciencesES45 papers
- University of GenevaCH45 papers
- Centre National de la Recherche ScientifiqueFR44 papers
- Institut d'Estudis Espacials de CatalunyaES44 papers
5 papers · 1 filter
Euclid: The convective-transition gap of 47 Tuc
M. Libralato, M. Griggio, R. Gerasimov +140
We report the first detection of the `convective-transition gap' (also known as `M-dwarf gap') in the globular cluster 47 Tuc (NGC 104) thanks to Euclid data. This feature, linked…
Gaia21bja: pre-main sequence star with quasi-periodic bursts
Ãdám Mátéfy, Zsófia Nagy, Ãgnes Kóspál +12
Gaia21bja is a Gaia alerted young stellar object (YSO) that exhibits at least seven quasi-peridoic brightenings over a 20 year-long light curve with durations of 1.5-2 years and am…
Correlation between active regions' spectra at high radio frequencies and solar flare occurrences
Sara Mulas, Alberto Pellizzoni, Marco Marongiu +31
High radio frequencies observations with the Italian network of large single-dish radio telescopes resulted in ~450 solar images between 2018 and 2023 in K-band frequency range (18…
A view of the evolution of a CME and the associated wave-trains at high spatial and temporal resolution
G. Russano, Y. De Leo, F. Frassati +13
Context. Studying the kinematic and dynamic evolution of fast eruptive events from the middle to high solar corona is a primary objective of the Metis coronagraph on Solar Orbiter.…
AT 2025abao: The fourth luminous red nova in M 31
A. Reguitti, A. Pastorello, G. Valerin +15
We present photometric and spectroscopic observations of the luminous red nova (LRN) AT 2025abao, the fourth discovered in M 31. The LRN, associated to the asymptotic giant branch…