POEMS SIGNED
Physics of Extreme Massive Stars
Total Cost €
0EC-Contrib. €
0Partnership
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0POEMS project word cloud
Explore the words cloud of the POEMS project. It provides you a very rough idea of what is the project "POEMS" about.
Project "POEMS" data sheet
The following table provides information about the project.
| Coordinator |
ASTRONOMICKY USTAV AV CR
Organization address contact info |
| Coordinator Country | Czech Republic [CZ] |
| Total cost | 952˙200 € |
| EC max contribution | 920˙000 € (97%) |
| Programme |
1. H2020-EU.1.3.3. (Stimulating innovation by means of cross-fertilisation of knowledge) |
| Code Call | H2020-MSCA-RISE-2018 |
| Funding Scheme | MSCA-RISE |
| Starting year | 2019 |
| Duration (year-month-day) | from 2019-01-01 to 2022-12-31 |
Partnership
Take a look of project's partnership.
| # | ||||
|---|---|---|---|---|
| 1 | ASTRONOMICKY USTAV AV CR | CZ (ONDREJOV) | coordinator | 455˙400.00 |
| 2 | TARTU ULIKOOL | EE (TARTU) | participant | 312˙800.00 |
| 3 | UNIVERSITY OF LEEDS | UK (LEEDS) | participant | 59˙800.00 |
| 4 | GEORG-AUGUST-UNIVERSITAT GOTTINGENSTIFTUNG OFFENTLICHEN RECHTS | DE (GOTTINGEN) | participant | 46˙000.00 |
| 5 | KONINKLIJKE STERRENWACHT VAN BELGIE | BE (BRUXELLES) | participant | 46˙000.00 |
| 6 | MINISTERIO DA CIENCIA, TECNOLOGIA, INOVAÇÕES E COMUNICAÇÕES | BR (BRASILIA) | partner | 0.00 |
| 7 | PONTIFICIA UNIVERSIDAD CATOLICA DE VALPARAISO | CL (VALPARAISO) | partner | 0.00 |
| 8 | SHAMAKHY ASTROPHYSICAL OBSERVATORYOF NATIONAL ACADEMY OF SCIENCES OF AZERBAIJAN | AZ (BAKU) | partner | 0.00 |
| 9 | UNIVERSIDAD DE VALPARAISO | CL (VALPARAISO) | partner | 0.00 |
| 10 | UNIVERSIDAD NACIONAL DE LA PLATA | AR (LA PLATA) | partner | 0.00 |
Map
Project objective
Massive stars are extreme cosmic engines, enriching their environments with chemically processed material throughout their entire life-time, and triggering star and planet formation. Despite their importance for the cosmic evolution, their evolutionary path up to their deaths as spectacular supernova explosions is most uncertain due to the lack of precise knowledge of the physical mechanisms behind mass eruptions. We wish to establish a multidisciplinary, international network of researchers from Europe, Asia, and South America with expertise in a variety of disciplines, and with background in both theory and observations. Our ultimate goal is to enlighten the processes that trigger mass loss in massive stars during extreme phases of their evolution. We will develop cutting-edge numerical codes suitable to describe the chemical and dynamical evolution of the stars, their winds, and their large-scale environments. In addition, we will initiate global observing campaigns utilizing facilities at major renowned observatories in combination with our national facilities, and exploit public archives from ground-based and space missions to acquire an outstanding set of urgently needed highest quality data. Confronting predictions from the numerical models with the observations will empower us to derive the first extensive and comprehensive set of precise physical parameters. The acquired results will significantly enhance our knowledge and lead to major advancements in all related fields. The bulk of exchanges will be undertaken by Early Stage Researchers and young Post-docs, who will be educated and trained in modern observing and data analyzing techniques and in high-performance computation, equipping them with excellent skills for their future careers. We will organize schools and workshops to share knowledge and to communicate and disseminate our results, which will be major breakthroughs and support the leading role of Europe in Astronomy.
Publications
| year | authors and title | journal | last update |
|---|---|---|---|
| 2019 |
J. KrtiÄka, J. JanÃk, I. KrtiÄková, S. Mereghetti, F. Pintore, P. Németh, J. Kubát, M. VuÄković Hot subdwarf wind models with accurate abundances published pages: A75, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201936208 |
Astronomy & Astrophysics 631 | 2020-01-29 |
| 2019 |
A. M. van Genderen, A. Lobel, H. Nieuwenhuijzen, G. W. Henry, C. de Jager, E. Blown, G. Di Scala, E. J. van Ballegoij Pulsations, eruptions, and evolution of four yellow hypergiants published pages: A48, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201834358 |
Astronomy & Astrophysics 631 | 2019-10-29 |
| 2019 |
C A H Condori, M Borges Fernandes, M Kraus, D Panoglou, C A Guerrero The study of unclassified B[e] stars and candidates in the Galaxy and Magellanic Clouds†published pages: 1090-1110, ISSN: 0035-8711, DOI: 10.1093/mnras/stz1540 |
Monthly Notices of the Royal Astronomical Society 488/1 | 2019-09-26 |
| 2019 |
Olga Maryeva, Roberto F. Viotti, Gloria Koenigsberger, Massimo Calabresi, Corinne Rossi, Roberto Gualandi The History Goes On: Century Long Study of Romano’s Star published pages: 79, ISSN: 2075-4434, DOI: 10.3390/galaxies7030079 |
Galaxies 7/3 | 2019-10-01 |
| 2019 |
Alex C. Gormaz-Matamala, M. Curé, L. S. Cidale, R. O. J. Venero Self-consistent Solutions for Line-driven Winds of Hot Massive Stars: The m-CAK Procedure published pages: 131, ISSN: 1538-4357, DOI: 10.3847/1538-4357/ab05c4 |
The Astrophysical Journal 873/2 | 2019-09-26 |
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