The Present and Future of Planetary Nebula Research. A White Paper by the IAU Planetary Nebula Working Group

Bibcode
2014RMxAA..50..203K
Kwitter, K. B.; Méndez, R. H.; Peña, M.; Stanghellini, L.; Corradi, R. L. M.; De Marco, O.; Fang, X.; Henry, R. B. C.; Karakas, A. I.; Liu, X.-W.; López, J. A.; Manchado, A.; Parker, Q. A.
Referencia bibliográfica

Revista Mexicana de Astronomía y Astrofísica Vol. 50, pp. 203-223 (2014)

Fecha de publicación:
10
2014
Número de autores
13
Número de autores del IAC
2
Número de citas
34
Número de citas referidas
29
Descripción
We present a summary of current research on planetary nebulae and their central stars, and related subjects such as atomic processes in ionized nebulae, AGB and post-AGB evolution. Future advances are discussed that will be essential to substantial improvements in our knowledge in the field.
Proyectos relacionados
Project Image
Nucleosíntesis y procesos moleculares en los últimos estados de la evolución estelar
Las estrellas de masa baja e intermedia (M < 8 masas solares, Ms) representan la mayoría de estrellas en el Cosmos y terminan sus vidas en la Rama Asintótica de las Gigantes (AGB) - justo antes de formar Nebulosas Planetarias (NPs) - cuando experimentan procesos nucleosintéticos y moleculares complejos. Las estrellas AGB son importantes
Domingo Aníbal
García Hernández
En ejecución
Tipo
Con árbitro
Sistema Solar y Sistemas Planetarios (SEYSS)
Física estelar e interestelar (FEEI)
La Vía Láctea y el Grupo Local (MWLG)
Nebulosas planetarias

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