Explore the words cloud of the StarFormMapper project. It provides you a very rough idea of what is the project "StarFormMapper" about.
The following table provides information about the project.
UNIVERSITY OF LEEDS
|Coordinator Country||United Kingdom [UK]|
|Total cost||1˙779˙602 €|
|EC max contribution||1˙775˙852 € (100%)|
1. H2020-EU.2.1.6. (INDUSTRIAL LEADERSHIP - Leadership in enabling and industrial technologies – Space)
|Duration (year-month-day)||from 2016-06-01 to 2020-05-31|
Take a look of project's partnership.
|1||UNIVERSITY OF LEEDS||UK (LEEDS)||coordinator||577˙892.00|
|2||QUASAR SCIENCE RESOURCES SL||ES (CANTOBLANCO)||participant||474˙732.00|
|3||CARDIFF UNIVERSITY||UK (CARDIFF)||participant||390˙727.00|
|4||UNIVERSITE GRENOBLE ALPES||FR (GRENOBLE)||participant||320˙000.00|
|5||UNIVERSITEIT LEIDEN||NL (LEIDEN)||participant||12˙500.00|
|6||UNIVERSITE GRENOBLE ALPES||FR (SAINT MARTIN D'HERES)||participant||0.00|
|7||UNIVERSITE JOSEPH FOURIER GRENOBLE 1||FR (GRENOBLE)||participant||0.00|
We propose to use a combination of data from the ESA space missions GAIA and Herschel, alongside other satellite and European-led ground-based observations, to map the density distribution of star formation regions. This will allow us to identify the mechanisms that underlie both how massive stars themselves form, but more fundamentally, how their natal clusters evolve around them. Our work will underpin studies of how all galaxies evolve. The combination of the two ESA missions will allow us to study clusters and associations of stars when they are very young (much less than 1 Myr old), when the structures we see are a better match to the initial conditions. No one has attempted such a project before as the required datasets were not available. The novel data and complexity of the combined datasets require the development of new analysis and visualization tools. In particular we will statistically compare hybrid large scale N-body SPH models with the combined 6-dimensional Gaia plus Herschel and gas kinematical data. Our goals therefore are structured to develop new techniques that we will initially test on simulations. We will follow this with tests on observational data of slightly older clusters (about 1Myr old). We will then apply the tested methodologies to the very youngest clusters. This will address our final goal of cracking the problem of how the most massive stars and clusters form.
|Data Management Plan update KO+40||Documents, reports||2020-02-25 17:32:25|
|Mass segregation methodology||Documents, reports||2020-02-25 17:32:25|
|Visualization client verification report||Documents, reports||2020-02-25 17:32:24|
|Clustering statistics report||Documents, reports||2020-02-25 17:32:25|
|Report on object catalogue from simulation data||Documents, reports||2020-02-25 17:32:24|
|Outreach activities report and plan KO+18||Documents, reports||2020-02-25 17:32:25|
|RISEA software library||Other||2020-02-25 17:32:24|
|Data Management Plan update KO+27||Documents, reports||2020-02-25 17:32:25|
|RISEA testing validation report||Documents, reports||2020-02-25 17:32:24|
|End of year 2 review||Documents, reports||2020-02-25 17:32:25|
|Revised SQAP v 2||Documents, reports||2020-02-25 17:32:25|
|Dissemination activities report and plan KO+18||Documents, reports||2020-02-25 17:32:24|
|Software Quality Assurance Plan||Documents, reports||2020-02-25 17:32:23|
|Substructure techniques||Documents, reports||2020-02-25 17:32:22|
|Gaia data architecture report||Documents, reports||2020-02-25 17:32:22|
|Virtualization study report||Documents, reports||2020-02-25 17:32:22|
|Outreach activities reports||Documents, reports||2020-02-25 17:32:23|
|Substructure software package||Other||2020-02-25 17:32:23|
|Report on available N-body simulations||Documents, reports||2020-02-25 17:32:24|
|Public project website||Websites, patent fillings, videos etc.||2020-02-25 17:32:23|
|Vizualisation server data resampling study||Documents, reports||2020-02-25 17:32:22|
|Additional observational data requirements||Documents, reports||2020-02-25 17:32:23|
|Report on Required Simulations||Documents, reports||2020-02-25 17:32:24|
|End of year 1 review||Documents, reports||2020-02-25 17:32:24|
|Data Management Plan v 1||Documents, reports||2020-02-25 17:32:24|
|Outreach activities update||Documents, reports||2020-02-25 17:32:23|
|Revised SQAP||Documents, reports||2020-02-25 17:32:23|
|RISEA architecture report||Documents, reports||2020-02-25 17:32:22|
Take a look to the deliverables list in detail: detailed list of StarFormMapper deliverables.
|year||authors and title||journal||last update|
F. Motte, T. Nony, F. Louvet, K. A. Marsh, S. Bontemps, A. P. Whitworth, A. Menâ€™shchikov, Q. Nguyá»…n LÆ°Æ¡ng, T. Csengeri, A. J. Maury, A. Gusdorf, E. Chapillon, V. KÃ¶nyves, P. Schilke, A. Duarte-Cabral, P. Didelon, M. Gaudel
The unexpectedly large proportion of high-mass star-forming cores in a Galactic mini-starburst
published pages: 478-482, ISSN: 2397-3366, DOI: 10.1038/s41550-018-0452-x
|Nature Astronomy 2/6||2020-02-25|
Phillip A B Galli, Isabelle Joncour, Estelle Moraux
Three-dimensional structure of the Upper Scorpius association with the Gaia first data release
published pages: L50-L54, ISSN: 1745-3933, DOI: 10.1093/mnrasl/sly036
|Monthly Notices of the Royal Astronomical Society: Letters 477/1||2020-02-25|
FrÃ©dÃ©rique Motte, Sylvain Bontemps, Fabien Louvet
High-Mass Star and Massive Cluster Formation in the Milky Way
published pages: 41-82, ISSN: 0066-4146, DOI: 10.1146/annurev-astro-091916-055235
|Annual Review of Astronomy and Astrophysics 56/1||2020-02-25|
J. Olivares, E. Moraux, L. M. Sarro, H. Bouy, A. Berihuete, D. Barrado, N. Huelamo, E. Bertin, J. Bouvier
The seven sisters DANCe
published pages: A70, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201731996
|Astronomy & Astrophysics 612||2020-02-25|
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The information about "STARFORMMAPPER" are provided by the European Opendata Portal: CORDIS opendata.
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