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Pre-perihelion evolution of the NiI/FeI abundance ratio in the coma of the interstellar comet 3I/ATLAS: From extreme to normal★

Emission lines of FeI and NiI are commonly found in the coma of Solar System comets, even at large heliocentric distances. These atoms are most likely released from the surface of the comet’s nucleus or from a short-lived parent. The presence of these lines in cometary spectra is unexpected because...

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Detalhes bibliográficos
Principais autores: Hutsemékers Damien, Manfroid Jean, Jehin Emmanuël, Opitom Cyrielle, Rahatgaonkar Rohan, Bannister Michele, Carvajal Juan Pablo, Dorsey Rosemary, Krishnakumar Aravind, Luco Baltasar, Murphy Brian, Puzia Thomas H.
Formato: Artigo
Idioma:Inglês
Publicado em: EDP Sciences 2026-02-01
Colecção:Astronomy & Astrophysics
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Acesso em linha:https://www.aanda.org/articles/aa/full_html/2026/02/aa57484-25/aa57484-25.html
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