Codice QR

Spectroscopic characterization of LOFAR radio-emitting M dwarfs

Recent observations with the LOw Frequency ARray (LOFAR) have revealed 19 nearby M dwarfs showing bright circularly polarized radio emission. One of the possible sources of such emission is through magnetic star-planet interactions (MSPIs) with unseen close-in planets. We present the initial results...

Descrizione completa

Salvato in:
Autori principali: Koo E., Stefansson G., Kavanagh R. D., Delamer M., Mahadevan S., Callingham J. R., Vedantham H., Robertson P., Bruijne D., Bender C. F., Cañas C. I., Diddams S., Espinoza-Retamal J. I., Fernandes R. B., Halverson S., Kanodia S., Krolikowski D., Lin A. S. J., Pope B. J. S., Roy A., Schwab C., Terrien R., Wright J. T.
Natura: Artigo
Lingua:Inglês
Pubblicazione: EDP Sciences 2026-02-01
Serie:Astronomy & Astrophysics
Soggetti:
techniques: radial velocities
techniques: spectroscopic
planets and satellites: fundamental parameters
planet-star interactions
binaries: spectroscopic
stars: low-mass
Accesso online:https://www.aanda.org/articles/aa/full_html/2026/02/aa56483-25/aa56483-25.html
Tags: Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!

Documenti analoghi