A sub-Neptune transiting the young field star HD 18599 at 40 pc

ABSTRACT Transiting exoplanets orbiting young nearby stars are ideal laboratories for testing theories of planet formation and evolution. However, to date only a handful of stars with age

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2023-04, Vol.522 (1), p.750-766
Hauptverfasser:	de Leon, J P, Livingston, J H, Jenkins, J S, Vines, J I, Wittenmyer, R A, Clark, J T, Winn, J I M, Addison, B, Ballard, S, Bayliss, D, Beichman, C, Benneke, B, Berardo, D A, Bowler, B P, Brown, T, Bryant, E M, Christiansen, J, Ciardi, D, Collins, K A, Collins, K I, Crossfield, I, Deming, D, Dragomir, D, Dressing, C D, Fukui, A, Gan, T, Giacalone, S, Gill, S, Gorjian, V, González Alvarez, E, Hesse, K, Horner, J, Howell, S B, Jenkins, J M, Kane, S R, Kendall, A, Kielkopf, J F, Kreidberg, L, Latham, D W, Liu, H, Lund, M B, Matson, R, Matthews, E, Mengel, M W, Morales, F, Mori, M, Narita, N, Nishiumi, T, Okumura, J, Plavchan, P, Quinn, S, Rabus, M, Ricker, G, Rudat, A, Schlieder, J, Schwarz, R P, Seager, S, Shporer, A, Smith, A M S, Stassun, K, Tamura, M, Tan, T G, Tinney, C, Vanderspek, R, Werner, M W, West, R G, Wright, D, Zhang, H, Zhou, G
Format:	Artikel
Sprache:	eng
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Zusammenfassung:	ABSTRACT Transiting exoplanets orbiting young nearby stars are ideal laboratories for testing theories of planet formation and evolution. However, to date only a handful of stars with age
ISSN:	0035-8711 1365-2966
DOI:	10.1093/mnras/stad894