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Global and local star formation with state-of-the-art physics

Objective

New stars form within large turbulent complexes harboring several thousands of solar masses of cold gas: the molecular clouds. The diffuse gas collapses gravitationally and heats up via compression until nuclear fusion reactions ignite and the star comes to life. The full description involves an intricate interplay between large-scale environmental factors and small-scale processes close to the star, connecting a number of physical mechanisms, including magnetic fields, self-gravity, radiative transfer, and time dependent chemistry.

The aim of the project is to construct a unified description of star formation, from large to small scales, using the world's most advanced numerical physics. A two-way approach will be used: the global approach (I) will deal with the dynamics of interstellar gas on the turbulent cloud scale, while the local approach (II) will concentrate on the formation of the protostellar seed.

The objectives are:

- Ia. Carry out a parameter study of the effects of cloud mass, turbulence, radiative transfer, and magnetization on stellar populations in giant molecular clouds
- Ib. Create a realistic model for protostellar radiative and outflow feedback and examine its effects on the star formation efficiency
- Ic. Quantify the effects of supernova-triggered star formation
- IIa. Simulate the formation of single protostars using extremely detailed physics (non-ideal MHD, multi-frequency radiative transfer)
- IIb. Incorporate for the first time into the simulations a chemistry module which interacts with the gas and radiation field
- IIc. Study episodic accretion events in protostars to try and explain under-luminous young stellar objects.

This is an ambitious, strongly multidisciplinary program, which fits perfecty in the research activities of the host institute. To ensure the project's success, I have a proven record of working with the different numerical techniques required, as well as an excellent understanding of astronomical observations.

Fields of science (EuroSciVoc)

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Programme(s)

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Topic(s)

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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.

MSCA-IF-EF-ST - Standard EF

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Call for proposal

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

(opens in new window) H2020-MSCA-IF-2014

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Coordinator

KOBENHAVNS UNIVERSITET
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 200 194,80
Address
NORREGADE 10
1165 KOBENHAVN
Denmark

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Region
Danmark Hovedstaden Byen København
Activity type
Higher or Secondary Education Establishments
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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.

€ 200 194,80
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