Workplans: workshop on planetary nebula observations
Entity
UAM. Departamento de Física TeóricaPublisher
MDPIDate
2020-03-16Citation
10.3390/galaxies8010023
Galaxies 8.1 (2020): 23
ISSN
2075-4434 (online)DOI
10.3390/galaxies8010023Funded by
I.A. acknowledges the support of Coordenação de Aperfeiçoamento de Pessoal de Nível Superior—Brasil (CAPES)—Finance Code 001. This research is supported by Space Telescope Science Institute grant HST-GO-15953.001-A to RIT (J.K.). T.U. was supported by NASA under grant NNX15AF24G issued through the Science Mission Directorate. E.V. acknowledges support from the “On the rocks II project” funded by the Spanish Ministerio de Ciencia, Innovación y Universidades under grant PGC2018-101950-B-I00. The Workshop was organized with the financial support of the Lorentz Center, which was provided by the Netherlands Organization for Scientific Research (NWO) and the Leiden UniversityEditor's Version
https://doi.org/10.3390/galaxies8010023Subjects
Planetary nebulae; Stars: evolution; Stars: late type; Stars: mass-loss; Stars: Winds and outflows; Stars: abundances; Plasmas; Dust; Extinction; Astrochemistry; FísicaRights
© 2020 by the authorsAbstract
This workshop is the second of the WORKPLANS series, which we started in 2016. The main
goal of WORKPLANS is to build up a network of planetary nebulae (PNe) experts to address the main
open questions in the field of PNe research. The specific aims of the WORKPLANS workshop series
are (i) to discuss and prioritize the most important topics to be investigated by the PN community in
the following years; (ii) to establish a network of excellent researchers with complementary expertise;
(iii) to formulate ambitious observing proposals for the most advanced telescopes and instrumentation
presently available (ALMA, SOFIA, VLT, GTC, HST, etc.), addressing those topics; and (iv) to develop
strategies for major proposals to future observatories (JWST, ELT, SPICA, Athena, etc.). To achieve
these goals, WORKPLANS II brought together experts in all key sub-areas of the PNe research field,
namely: analysis and interpretation of PNe observational data; theoretical modeling of gas and
dust emission; evolution from Asymptotic Giant Branch stars (PNe progenitors) to PNe; and the
instrumentation and technical characteristics of the relevant observatories
Files in this item
Google Scholar:Aleman, Isabel
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Bernard-Salas, Jeronimo
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Kastner, Joel H
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Ueta, Toshiya
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Villaver Sobrino, Eva Gloria
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