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Horizon 2020 project information and now also report summaries are available on CORDIS. All H2020 projects can be downloaded from the EU Open Data Portal .

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Evolved stars: clues to the chemical evolution of galaxies
ID: 269193
Start date: 2011-04-01, End date: 2015-03-31
The late stages in the evolution of intermediate-mass stars (Asymptotic Giant Branch - AGB and post-AGB) are of the greatest importance for the chemical evolution of galaxies. Pulsations, dust formation, and mass loss through massive stellar winds are characteristic phenomena...
Programme: FP7-PEOPLE
Record Number: 98689
Last updated on: 2017-05-29
Final Report Summary - POSTAGBINGALAXIES (Evolved stars: clues to the chemical evolution of galaxies)
The late stages (Asymptotic Giant Branch - AGB and post-AGB) of the life of intermediate-mass stars are of the greatest importance for the chemical evolution of galaxies. Pulsations, dust formation, and mass loss through massive stellar winds are characteristic phenomena for...
Programme: FP7-PEOPLE
Record Number: 171706
Last updated on: 2015-10-20
Evolución de las estrellas en la rama asintótica gigante
La última fase de las estrellas cuya masa es varias veces la del Sol es la rama asintótica gigante (RAG). Científicos financiados con fondos de la Unión Europea estudiaron el superviento de la atmósfera de estas estrellas para desentrañar su función en la ecología galáctica.
Programme: FP7-PEOPLE
Record Number: 181003
Last updated on: 2016-04-12
Available languages: DE, EN, ES, FR, IT, PL
Evolution of asymptotic giant branch stars
For stars a few times more massive than our Sun, the last phase in their evolution is the asymptotic giant branch (AGB). EU-funded scientists looked into the superwind of these stars' atmospheres to elucidate their role in the galactic ecology.
Programme: FP7-PEOPLE
Record Number: 181003
Last updated on: 2016-04-12
Available languages: DE, EN, ES, FR, IT, PL
Die Entwicklung von AGB-Sternen
Bei Sternen, deren Masse ein Mehrfaches unserer Sonne beträgt, endet die Entwicklung mit der AGB (asymptotic giant branch) -Phase EU-finanzierte Wissenschaftler untersuchten den Superwind in den Atmosphären dieser Sterne, um deren Bedeutung für die galaktische Ökologie zu beleuchten.
Programme: FP7-PEOPLE
Record Number: 181003
Last updated on: 2016-04-12
Available languages: DE, EN, ES, FR, IT, PL
Evoluzione delle stelle del ramo asintotico delle giganti
Per le stelle che sono alcune volte più massive rispetto al nostro Sole, l’ultima fase nella loro evoluzione è il ramo asintotico delle giganti (AGB, asymptotic giant branch). Scienziati finanziati dall’UE hanno esaminato il supervento delle atmosfere di queste stelle per chiarire il suo ruolo nell’ecologia galattica.
Programme: FP7-PEOPLE
Record Number: 181003
Last updated on: 2016-04-12
Available languages: DE, EN, ES, FR, IT, PL
L'évolution des étoiles asymptotiques à branches géantes
Pour les étoiles quelques fois plus massives que notre soleil, la dernière phase de leur évolution est la branche géante asymptotique (BGA). Des scientifiques financés par l'UE ont étudié le super-vent des atmosphères de ces étoiles pour élucider leur rôle dans l'écologie galactique.
Programme: FP7-PEOPLE
Record Number: 181003
Last updated on: 2016-04-12
Available languages: DE, EN, ES, FR, IT, PL
Ewolucja gwiazd AGB
[RESULT IN BRIEF] Ewolucja gwiazd AGB
W przypadku gwiazd o masie kilkakrotnie większej od masy Słońca, ostatnią fazą ewolucji jest przemiana w gwiazdę na asymptotycznej gałęzi olbrzymów, tzw. gwiazdę AGB. Wspierani ze środków UE badacze przyjrzeli się zjawisku tzw. superwiatru, występującemu w atmosferze tych gwiazd, aby wyjaśnić ich rolę w ekologii galaktycznej.
Programme: FP7-PEOPLE
Record Number: 181003
Last updated on: 2016-04-12
Available languages: DE, EN, ES, FR, IT, PL
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List retrieved on: 2017-06-25