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POEMS SIGNED

Physics of Extreme Massive Stars

Total Cost €

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EC-Contrib. €

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Partnership

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 POEMS 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.

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Project "POEMS" data sheet

The following table provides information about the project.

Coordinator
ASTRONOMICKY USTAV AV CR 

Organization address
address: FRICOVA 298
city: ONDREJOV
postcode: 25165
website: www.asu.cas.cz

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 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.

# participants  country  role  EC contrib. [€] 
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
List of publications.
2019 J. Krtička, J. Janík, I. Krtičková, S. Mereghetti, F. Pintore, P. Németh, J. Kubát, M. Vučković
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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