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Long-term activity cycles in planetary M stars observed with SOPHIE

Context. M dwarfs are prime targets for exoplanet searches due to their low masses and radii, which enable the detection of small planets in their habitable zones (HZs). However, the magnetic activity of M dwarfs can introduce signals in radial velocity measurements that may be mistaken for planetar...

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Egile Nagusiak: Oviedo C. G., Buccino A. P., Díaz R. F., Petrucci R., Jofré E., Boisse I., Colombo P. D., Delfosse X.
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: EDP Sciences 2026-04-01
Saila:Astronomy & Astrophysics
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Sarrera elektronikoa:https://www.aanda.org/articles/aa/full_html/2026/04/aa56087-25/aa56087-25.html
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