The Missing Link: Unlocking galaxy evolution by understanding star formation.
Lead Research Organisation:
University of Manchester
Department Name: Physics and Astronomy
Abstract
Stars are the engines that drive how galaxies evolve. When massive stars die the resulting supernova explosions transfer energy to the gas in the galaxy and support it against gravitational collapse. Stars form all the elements heavier than Helium by nuclear fusion, and these elements are returned to the galaxy in the supernova explosions. Planets are formed as by-products of star-formation, and the energy that they emit may fuel life on those planets. An understanding of how stars form is crucial to understanding the evolution of galaxies since the Big Bang. We can test this process using revolutionary new telescopes like the Atacama Large Millimetre and sub-millimetre Array (ALMA) and the future Square Kilometre Array (SKA). These advanced facilities will make it possible to observe the different environments within other galaxies in unprecedented detail.
To solve the mystery of how stars form in other galaxies we will first need good predictions that can be compared against the observations. I want to help solve this mystery by using supercomputer simulations to create extremely detailed models of where gas is concentrated into clouds in different types of galaxies. These gas clouds are known as molecular clouds, because they mainly consist of hydrogen molecules, and are the stellar nurseries in which stars are born. I will use the models to predict the temperature, density, chemical composition, and gas motions, and then investigate how easily the gas collapses to form stars, the type of stars formed, and the numbers of stars in the different clouds. This will enable me to determine whether molecular clouds and the stars formed in them are the same everywhere, or whether they vary with galactic environment. This is an important assumption as in observations we can only see the very brightest stars in other galaxies and have to assume that the fainter stars form in the same proportion as we see in nearby star-forming regions in our own Milky-Way Galaxy.
Previous models of star-formation always started with simple estimates of how clouds might begin, but uniquely, this project uses actual galaxy models. A major innovation is that I will use a chemical model to predict the composition of the gas, which will determine the emission seen by a telescope. For example, ALMA is sensitive to the emission from carbon monoxide gas, and the SKA will be sensitive to emission from atomic hydrogen. Using the computer simulations generated from this project I will make synthetic observations of the molecular clouds in other galaxies. In other galaxies we know that the amount of gas, the structure of the galaxy, and the chemical composition may be different, and so how clouds appear when observed will also be different. We can compare the computer generated emission maps to the observed maps as a reference guide to determine what the properties of the observed clouds actually are. Astronomical observations are 2D projected images of what are 3D structures, moreover, the emitted light changes with the temperature and density of the gas. This makes molecular clouds hard to understand without a good model to compare against. This is particularly true of modern telescopes as due to their improved resolution and sensitivity the observations are very complex due to the fine details that they can see. Consequently, the models from this project will be crucial in using ALMA and the SKA to determine how stars form throughout our Universe.
To solve the mystery of how stars form in other galaxies we will first need good predictions that can be compared against the observations. I want to help solve this mystery by using supercomputer simulations to create extremely detailed models of where gas is concentrated into clouds in different types of galaxies. These gas clouds are known as molecular clouds, because they mainly consist of hydrogen molecules, and are the stellar nurseries in which stars are born. I will use the models to predict the temperature, density, chemical composition, and gas motions, and then investigate how easily the gas collapses to form stars, the type of stars formed, and the numbers of stars in the different clouds. This will enable me to determine whether molecular clouds and the stars formed in them are the same everywhere, or whether they vary with galactic environment. This is an important assumption as in observations we can only see the very brightest stars in other galaxies and have to assume that the fainter stars form in the same proportion as we see in nearby star-forming regions in our own Milky-Way Galaxy.
Previous models of star-formation always started with simple estimates of how clouds might begin, but uniquely, this project uses actual galaxy models. A major innovation is that I will use a chemical model to predict the composition of the gas, which will determine the emission seen by a telescope. For example, ALMA is sensitive to the emission from carbon monoxide gas, and the SKA will be sensitive to emission from atomic hydrogen. Using the computer simulations generated from this project I will make synthetic observations of the molecular clouds in other galaxies. In other galaxies we know that the amount of gas, the structure of the galaxy, and the chemical composition may be different, and so how clouds appear when observed will also be different. We can compare the computer generated emission maps to the observed maps as a reference guide to determine what the properties of the observed clouds actually are. Astronomical observations are 2D projected images of what are 3D structures, moreover, the emitted light changes with the temperature and density of the gas. This makes molecular clouds hard to understand without a good model to compare against. This is particularly true of modern telescopes as due to their improved resolution and sensitivity the observations are very complex due to the fine details that they can see. Consequently, the models from this project will be crucial in using ALMA and the SKA to determine how stars form throughout our Universe.
Publications
Barnes A
(2023)
PHANGS-JWST First Results: Multiwavelength View of Feedback-driven Bubbles (the Phantom Voids) across NGC 628
in The Astrophysical Journal Letters
Beuther H
(2016)
The HI/OH/Recombination line survey of the inner Milky Way (THOR) Survey overview and data release 1???
in Astronomy & Astrophysics
Beuther H
(2020)
Gravity and Rotation Drag the Magnetic Field in High-mass Star Formation
in The Astrophysical Journal
Beuther H
(2018)
Magnetic fields at the onset of high-mass star formation
in Astronomy & Astrophysics
Beuther H.
(2018)
Magnetic fields at the onset of high-mass star formation
in ArXiv e-prints
Bihr S
(2017)
Kinematic and thermal structure at the onset of high-mass star formation - ISOSS23053
in Proceedings of the International Astronomical Union
Bonnell I
(2014)
The Labyrinth of Star Formation
Eibensteiner C
(2023)
Kinematic analysis of the super-extended H I disk of the nearby spiral galaxy M 83
in Astronomy & Astrophysics
Feng S
(2016)
Are infrared dark clouds really quiescent?
in Astronomy & Astrophysics
Ginsburg A
(2016)
Toward gas exhaustion in the W51 high-mass protoclusters
in Astronomy & Astrophysics
Description | Astrophysics and Cosmology Research at the Jodrell Bank Centre for Astrophysics 2023-2026 |
Amount | £3,874,951 (GBP) |
Funding ID | ST/X001229/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 04/2023 |
End | 03/2026 |
Description | RADA: Radio Astronomy for Development in the Americas |
Amount | £40,277 (GBP) |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 09/2018 |
End | 08/2019 |
Description | SKA postgraduate exchange program 2017 |
Amount | £40,000 (GBP) |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 05/2018 |
End | 05/2020 |
Title | PCA Factory |
Description | A new open source module, which smartly performs PCA to extract velocity structure functions from simulated or real data of the ISM in a user-friendly way. Software DOI: 10.5281/zenodo.3822718 |
Type Of Material | Data analysis technique |
Year Produced | 2021 |
Provided To Others? | Yes |
Impact | This was developed as part of a major publication meeting one of the key goals of the project, to compare to CO line observations in the observational space. |
URL | http://github.com/andizq/pcafactory |
Title | Synthetic Large-scale Galactic Filaments: On Their Formation, Physical Properties, and Resemblance to Observations |
Description | Publicly available grid of models representing the Interstellar Medium at galactic scales. |
Type Of Material | Database/Collection of data |
Year Produced | 2019 |
Provided To Others? | Yes |
Impact | Dataset was the basis of a publication and enabled a comparison between several observational studies and theoretical data. |
URL | https://dataverse.harvard.edu/ |
Description | CARMA NRAO Orion survey |
Organisation | Yale University |
Department | Department of Physics |
Country | United States |
Sector | Academic/University |
PI Contribution | Participation in team telecoms discussing results. Feedback on paper drafts. |
Collaborator Contribution | A large CO survey of Orion. |
Impact | 1st paper submitted. |
Start Year | 2016 |
Description | ECOGAL |
Organisation | Heidelberg University |
Country | Germany |
Sector | Academic/University |
PI Contribution | Member of the large-scale working group investigating how star formation and galactic structure is linked using Arepo simulations of the galactic ISM. |
Collaborator Contribution | An international team focussed between Germany, France and Italy with Manchester in the UK. The main focus is the galactic ecosystem of star formation. |
Impact | No outcomes to report as yet. |
Start Year | 2022 |
Description | PHANGS |
Organisation | Max Planck Society |
Department | Max Planck Institute for Astronomy |
Country | Germany |
Sector | Academic/University |
PI Contribution | Physics at High Angular Resolution in Nearby Galaxies Survey Lead by Prof Eva Schinerer at the MPIA with collaborators throughout Europe and the US. I provide theoretical modelling and comparison to the observed data as well as contributing to group discussions and paper revision. |
Collaborator Contribution | The collaboration is the world leading survey of the resolved ISM in nearby galaxies. |
Impact | JWST special edition in ApJL |
Start Year | 2022 |
Description | THOR collaboration |
Organisation | Max Planck Society |
Department | Max Planck Institute for Astronomy |
Country | Germany |
Sector | Academic/University |
PI Contribution | Member of the collaboration team. Help in preparation of papers. |
Collaborator Contribution | THOR is a collaboration studying the "The HI, OH, Recombination line survey of the Milky Way. |
Impact | 1 paper published and the 2nd in final stages of review. |
Start Year | 2015 |
Description | The hunt for Nessie |
Organisation | Harvard University |
Department | Harvard-Smithsonian Center for Astrophysics |
Country | United States |
Sector | Academic/University |
PI Contribution | Providing a theoretical dataset of simulated Milky Way clouds. |
Collaborator Contribution | Comparing the simulations to observed Galactic filaments using the same techniques as in their observations. |
Impact | None as yet. |
Start Year | 2017 |
Description | I'm a Scientist get me out of here |
Form Of Engagement Activity | Engagement focused website, blog or social media channel |
Part Of Official Scheme? | No |
Geographic Reach | National |
Primary Audience | Schools |
Results and Impact | Live text-chat with school pupils as part of the Pink Zone on the I'm a Scientist Website throughout the month of March 2021. |
Year(s) Of Engagement Activity | 2021 |
Description | Meet the Expert Talk - Jodrell Bank Discovery Centre |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | Public talk during school half terms describing my work and answering astronomy questions from the audience at the Jodrell Bank Discovery Centre. |
Year(s) Of Engagement Activity | 2017 |