A circumbinary planet in orbit around the short-period white dwarf eclipsing binary RR cae

By using six newly determined mid-eclipse times together with those collected from the literature, we have found that the observed minus calculated (O-C) curve of RR Cae shows a cyclic change with a period of 11.9yr and an amplitude of 14.3 s while it undergoes an upward parabolic variation [reveali...

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Detalles Bibliográficos
Autores principales:	Qian, S. B., Liu, L., Zhu, L. Y., Dai, Z. B., Fernández Lajús, Eduardo, Baume, Gustavo
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2012
Materias:	Ciencias Astronómicas Binaries: close Binaries: eclipsing Planetary systems Stars: individual: RR cae White dwarfs
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/84385
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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