##plugins.themes.healthSciences.language.toggle##
Español
Inglés
##navigation.register##
##navigation.login##
Actual
Archivo
##navigation.about##
##about.aboutContext##
##about.editorialTeam##
##manager.setup.privacyStatement##
##about.contact##
Instrucciones para autores y editores especiales
##common.search##
RmXAA
##navigation.register##
##navigation.login##
##plugins.themes.healthSciences.language.toggle##
Español
Inglés
Vol. 15 Núm. 1 (2003)
,
Contributions
Vol. 15 Núm. 1 (2003)
Contributions
A Dynamical Model for PNe with WR-Type Central Stars
Medina S.
+
−
García-Segura G.
+
−
Peña M.
+
−
Medina S.
Instituto de Astronomía, Universidad Nacional Autó-noma de México, Apartado Postal 70-264, 04510 Mé-xi-co, D. F., Mé-xi-co
García-Segura G.
-
Peña M.
-
PDF (Inglés)
PDF (Inglés)
Palabras clave
ISM: Kinematics and dynamics
Planetary Nebulae: General
Stars: AGB and post-AGB
##submission.howToCite##
A Dynamical Model for PNe with WR-Type Central Stars. (2003).
Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias
,
15
(1), 78-78.
https://astronomia.unam.mx/journals/rmxac/article/view/2003rmxac..15...78m
hola
##submission.howToCite.citationFormats##
##plugins.generic.citationStyleLanguage.style.acm-sig-proceedings##
##plugins.generic.citationStyleLanguage.style.acs-nano##
##plugins.generic.citationStyleLanguage.style.apa##
##plugins.generic.citationStyleLanguage.style.associacao-brasileira-de-normas-tecnicas##
##plugins.generic.citationStyleLanguage.style.chicago-author-date##
##plugins.generic.citationStyleLanguage.style.harvard-cite-them-right##
##plugins.generic.citationStyleLanguage.style.ieee##
##plugins.generic.citationStyleLanguage.style.modern-language-association##
##plugins.generic.citationStyleLanguage.style.turabian-fullnote-bibliography##
##plugins.generic.citationStyleLanguage.style.vancouver##
##plugins.generic.citationStyleLanguage.style.ama##
##submission.howToCite.downloadCitation##
##plugins.generic.citationStyleLanguage.download.ris##
##plugins.generic.citationStyleLanguage.download.bibtex##
Resumen
In this work we present the preliminary results of a dynamical analysis on a homogeneously observed sample consisting of 21 planetary nebulae with central stars of the [WC] type (WRPNe) from the list of Tylenda, Acker, & Stendholm (1993).
×
##user.username##
*
##common.required##
##user.password##
*
##common.required##
##user.login.forgotPassword##
##user.login.rememberUsernameAndPassword##
##user.login##
##plugins.themes.healthSciences.register.noAccount##
##plugins.themes.healthSciences.register.registerHere##