K. B. Kwitter1, R. H. Méndez2, M. Peña3, L. Stanghellini4, R. L. M. Corradi5,6, O. De Marco7, X. Fang8,9, R. B. C. Henry10, A. I. Karakas11, X.-W. Liu8,9, J. A. Lopez12, A. Manchado5,6, and Q. A. Parker7
1 Department of Astronomy, Williams College, 33 Lab Campus Drive, Williamstown, MA 01267, USA (Karen.B.Kwitter@williams.edu).
2 Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA (mendez@ifa.hawaii.edu).
3 Instituto de Astronomía, Universidad Nacional Autónoma de México, 04510 México, D.F., México (miriam@astro.unam.mx).
4 National Optical Astronomy Observatory, 950 N. Cherry Ave., Tucson, AZ 85719, USA (lstanghellini@noao.edu).
5 Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain (rcorradi, amt@iac.es).
]]> 6 Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain (rcorradi, amt@iac.es).7 Department of Physics & Astronomy, Macquarie University, Sydney, NSW 2109, Australia (orsola.demarco, quentin.parker@mq.edu.au).
8 Department of Astronomy, School of Physics, Peking University, Beijing 100871, China (fangx@iaa.es, x.liu@pku.edu.cn).
9 Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China (fangx@iaa.es, x.liu@pku.edu.cn).
10 H.L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019, USA (henry@nhn.ou.edu).
11 Research School of Astronomy & Astrophysics, Mt. Stromlo Observatory, Weston Creek ACT 2611, Australia (akarakas@mso.anu.edu.au).
12 Instituto de Astronomía, Universidad Nacional Autónoma de México, Campus Ensenada, Ensenada, B.C., México (jal@astrosen.unam.mx).
Received 2014 January 22.
Accepted 2014 March 21.
RESUMEN
Se presenta un resumen del estado actual de la investigación sobre las nebulosas planetarias y sus estrellas centrales, y temas relacionados como los procesos atómicos en nebulosas ionizadas, y la evolución de las estrellas de la rama gigante asintótica y post-gigante asintótica. Se discuten los avances futuros que serán necesarios para incrementar sustancialmente nuestro conocimiento en este campo.
ABSTRACT
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.
Key Words: ISM: abundances — planetary nebulae: general — stars: AGB and post-AGB — stars: evolution.
DESCARGAR ARTÍCULO EN FORMATO PDF
]]> REFERENCES
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