Skip to main content
Go to the home page of the European Commission (opens in new window)
English en
CORDIS - EU research results
CORDIS
Content archived on 2024-05-28

Coordinated Observational and Numerical Studies of InterStellar Tracers

Objective

The dynamical and chemical evolution of diffuse interstellar gas is a key process in the development of structure in the Universe, leading to the subsequent production of stars, planets and ultimately, life itself. The goals of this research programme are to bring together the most comprehensive, detailed astrophysical data of the neutral phases of the interstellar medium in our Galaxy and the most complete current model of their dynamical and evolutionary relationship. Our observational data are from new, forefront international observational initiatives at multiple wavelengths, while our numerical magnetohydrodynamic models of our entire Galaxy uniquely include spiral structure, multi-temperature and multi-phase capability through the addition of CO and H2 formation from the atomic gas. The key advances enabled by the numerical models are the ability to visualize and quantify the time evolution of important ISM structures (e.g. molecular clouds) and reveal the observationally invisible molecular hydrogen component. The models provide context for understanding the observational signatures of particular stages of evolution (e.g. HI self-absorption clouds, infrared dark clouds) that are of current great scientific interest. The detailed observational data in turn allow tests of the spiral shock model of molecular cloud formation (thought to be the dominant evolutionary path) in terms of (e.g.) the kinematic structure of CO and HI emission, the amount of HISA produced for given model parameters, the reproduction of the molecular cloud size-linewidth relation, and other measures. There are many avenues for the development of this core research, both observationally and theroretically, that will extend beyond the nominal duration of the project. The models and data together will form the basis of a virtuous cycle, wherein refinements and extensions to the models are imposed by the data.

Fields of science (EuroSciVoc)

CORDIS classifies projects with EuroSciVoc, a multilingual taxonomy of fields of science, through a semi-automatic process based on NLP techniques. See: The European Science Vocabulary.

You need to log in or register to use this function

Keywords

Project’s keywords as indicated by the project coordinator. Not to be confused with the EuroSciVoc taxonomy (Fields of science)

Topic(s)

Calls for proposals are divided into topics. A topic defines a specific subject or area for which applicants can submit proposals. The description of a topic comprises its specific scope and the expected impact of the funded project.

Call for proposal

Procedure for inviting applicants to submit project proposals, with the aim of receiving EU funding.

FP7-PEOPLE-2007-4-2-IIF
See other projects for this call

Funding Scheme

Funding scheme (or “Type of Action”) inside a programme with common features. It specifies: the scope of what is funded; the reimbursement rate; specific evaluation criteria to qualify for funding; and the use of simplified forms of costs like lump sums.

MC-IIF - International Incoming Fellowships (IIF)

Coordinator

THE UNIVERSITY OF EXETER
EU contribution
€ 170 709,11
Address
THE QUEEN'S DRIVE NORTHCOTE HOUSE
EX4 4QJ Exeter
United Kingdom

See on map

Region
South West (England) Devon Devon CC
Activity type
Higher or Secondary Education Establishments
Links
Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

No data
My booklet 0 0