Star formation (SF) has been continuous since the Universe was 200 million years old. It occurs in the interstellar medium (ISM) – the gas and dust between stars within galaxies. The majority of SF occurs inside giant molecular clouds (GMCs) – the most massive agglomerations of dense gas within the ISM – typically the stars form in clusters. Initially the SF is governed solely by a GMC’s morphology, but, as stars form, the energy and momentum they inject into their surroundings – stellar feedback – affects ongoing star formation within the GMC. The effects of this feedback not only help to break up the cloud, but affect the wider ISM, and hence influence both neighbouring GMC evolution and future GMC formation. This thesis explores how two ...
It is a major open question which physical processes stop gas accretion on to giant molecular clouds...
Massive stars, with a mass more than 8 Solar-masses, have a strong destructive impact on the clouds ...
Massive stars, with a mass more than 8 Solar-masses, have a strong destructive impact on the clouds ...
Stars and the gas between them - the interstellar medium - are intrinsically coupled. Massive stars ...
This is the author accepted manuscript. The final version is available from Oxford University Press ...
We present here the first of a series of papers aimed at better understanding the evolution and prop...
This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Noti...
Many uncertainties remain as to how the most massive stars are formed and how they interact with the...
Feedback -- from stars and supermassive black holes -- is the bottleneck of our understanding on gal...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
IAB acknowledges funding from the European Research Council for the FP7 ERC advanced grant project E...
We have used the AMR hydrodynamic code, MG, to perform 3D hydrodynamic simulations with self-gravity...
In this thesis we address the problem of understanding the star formation process in giant molecular...
We develop and implement numerical methods for including stellar feedback in galaxy-scale numerical ...
IAB acknowledges funding from the European Research Council for the FP7 ERC advanced grant project E...
It is a major open question which physical processes stop gas accretion on to giant molecular clouds...
Massive stars, with a mass more than 8 Solar-masses, have a strong destructive impact on the clouds ...
Massive stars, with a mass more than 8 Solar-masses, have a strong destructive impact on the clouds ...
Stars and the gas between them - the interstellar medium - are intrinsically coupled. Massive stars ...
This is the author accepted manuscript. The final version is available from Oxford University Press ...
We present here the first of a series of papers aimed at better understanding the evolution and prop...
This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Noti...
Many uncertainties remain as to how the most massive stars are formed and how they interact with the...
Feedback -- from stars and supermassive black holes -- is the bottleneck of our understanding on gal...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
IAB acknowledges funding from the European Research Council for the FP7 ERC advanced grant project E...
We have used the AMR hydrodynamic code, MG, to perform 3D hydrodynamic simulations with self-gravity...
In this thesis we address the problem of understanding the star formation process in giant molecular...
We develop and implement numerical methods for including stellar feedback in galaxy-scale numerical ...
IAB acknowledges funding from the European Research Council for the FP7 ERC advanced grant project E...
It is a major open question which physical processes stop gas accretion on to giant molecular clouds...
Massive stars, with a mass more than 8 Solar-masses, have a strong destructive impact on the clouds ...
Massive stars, with a mass more than 8 Solar-masses, have a strong destructive impact on the clouds ...