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The scatter of the M dwarf mass-radius relationship

Autor
Parsons, S.; Gänsicke, B. T.; Marsh, T.; Rebassa, A.
Tipus d'activitat
Article en revista
Revista
Montly Notices of the Royal Astronomical Society
Data de publicació
2018-11-21
Volum
481
Número
1
Pàgina inicial
1083
Pàgina final
1096
DOI
https://doi.org/10.1093/MNRAS/STY2345 Obrir en finestra nova
Projecte finançador
Ajut per a contractació RYC-2016-20254
Del enfriamiento a las explosiones: la física de los objetos compactos
Grup d'astronomia i astrofísica
Repositori
http://hdl.handle.net/2117/127463 Obrir en finestra nova
URL
https://academic.oup.com/mnras/article-abstract/481/1/1083/5079656 Obrir en finestra nova
Resum
M dwarfs are prime targets in the hunt for habitable worlds around other stars. This is due to their abundance as well as their small radii and low masses and tempera- tures, which facilitate the detection of temperate, rocky planets in orbit around them. However, the fundamental properties of M dwarfs are difficult to constrain, often lim- iting our ability to characterise the planets they host. Here we test several theoretical relationships for M dwarfs by measuring 23 high precision, model-in...
Citació
Parsons, S., Gänsicke, B. T., Marsh, T., Rebassa, A. The scatter of the M dwarf mass-radius relationship. "Montly Notices of the Royal Astronomical Society", 21 Novembre 2018, vol. 481, núm. 1, p. 1083-1096.
Paraules clau
Binaries - eclipsing, Stars - fundamental parameters, Stars - late-type
Grup de recerca
GAA - Grup d'Astronomia i Astrofísica

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