Transition disks: Four candidates for ongoing giant planet formation in Ophiuchus

Mostrar todas las versiones(3)

Among the large set of Spitzer-selected transitional disks that we have examined in the Ophiuchus molecular, four disks have been identified as (giant) planet-forming candidates based on the morphology of their spectral energy distributions (SEDs), their apparent lack of stellar companions, and evid...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Orellana, M., Cieza, L.A., Schreiber, M.R., Merín, B., Brown, J.M., Pellizza, L.J., Romero, G.A.
Formato: JOUR
Materias:
protoplanetary disks
stars: pre-main sequence
submillimeter: planetary systems
Best-fit model parameters
Density profile
Dust distribution
Dust settling
Giant planet formation
Giant planets
Inner cavities
MONTE CARLO
Monte Carlo Markov chain
Parameter spaces
Parameter values
Parametric models
Protoplanetary disks
Spectral energy distribution
Statistical confidence
Submillimeter: planetary systems
Temperature structure
Thermal equilibriums
Grain growth
Stars
Dust
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v539_n_p_Orellana
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

Ejemplares similares

Ejemplares similares