Accretion of clumpy cold gas onto massive black hole binaries: a possible fast route to binary coalescence

dc.creatorGarrido Goicovic, Felipe
dc.creatorMaureira-Fredes, Cristian
dc.creatorSesana, Alberto
dc.creatorAmaro-Seoane, Pau
dc.creatorCuadra, Jorge
dc.date.accessioned2020-01-20T19:36:04Z
dc.date.available2020-01-20T19:36:04Z
dc.date.created2020-01-20T19:36:04Z
dc.date.issued2018
dc.identifier10.1093/mnras/sty1709
dc.identifier0035-8711
dc.identifierhttps://doi.org/10.1093/mnras/sty1709
dc.identifierhttps://repositorio.uc.cl/handle/11534/27667
dc.languageen
dc.subjectaccretion, accretion discs
dc.subjectblack hole physics
dc.subjecthydrodynamics
dc.subjectgalaxies: evolution
dc.subjectgalaxies: nuclei
dc.titleAccretion of clumpy cold gas onto massive black hole binaries: a possible fast route to binary coalescence
dc.typeartículo


Este ítem pertenece a la siguiente institución