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Open AccessEditorial

WORKPLANS: Workshop on Planetary Nebula Observations

1
Instituto de Física e Química, Universidade Federal de Itajubá, Av. BPS 1303, Pinheirinho, Itajubá 37500-903, Brazil
2
ACRI-ST, 260 Route du Pin Montard, 06904 Sophia-Antipolis, France
3
Center for Imaging Science, School of Physics and Astronomy, and Laboratory for Multiwavelength Astrophysics, Rochester Institute of Technology, 54 Lomb Memorial Drive, Rochester, NY 14623, USA
4
Department of Physics & Astronomy, University of Denver, 2112 E. Wesley Ave., Denver, CO 80208, USA
5
Departamento de Física Teórica, Universidad Autóonoma de Madrid, 28049 Madrid, Spain
*
Author to whom correspondence should be addressed.
Workshop scientific organizers. These authors contributed equally to this work.
Galaxies 2020, 8(1), 23; https://doi.org/10.3390/galaxies8010023
Received: 27 February 2020 / Accepted: 5 March 2020 / Published: 16 March 2020
(This article belongs to the Special Issue Workplans II: Workshop for Planetary Nebula Observations)
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. View Full-Text
Keywords: planetary nebulae; stars: evolution; stars: late type; stars: mass-loss; stars: winds and outflows; stars: abundances; plasmas; dust; extinction; astrochemistry planetary nebulae; stars: evolution; stars: late type; stars: mass-loss; stars: winds and outflows; stars: abundances; plasmas; dust; extinction; astrochemistry
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Aleman, I.; Bernard-Salas, J.; Kastner, J.H.; Ueta, T.; Villaver, E. WORKPLANS: Workshop on Planetary Nebula Observations. Galaxies 2020, 8, 23.

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