Modelling radiative feedback in star forming regions

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Jul 10, 2013 ... Mind The Gap, Cambrige -. 08/07/2013. Modelling radiative feedback in star forming regions. Thomas Haworth. Tim Harries, David Acreman.
Modelling radiative feedback in star forming regions

Thomas Haworth Tim Harries, David Acreman Mind The Gap, Cambrige 08/07/2013 Wednesday, 10 July 13

Bonnell + (2013), 430, 1790

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Mind The Gap, Cambrige 08/07/2013 Wednesday, 10 July 13

Bonnell + (2013), 430, 1790

IC1848 Spitzer Mind The Gap, Cambrige 08/07/2013 Wednesday, 10 July 13

TORUS is a state of the art radiation transport code with a hydrodynamics module bolted on.

• Adaptive mesh refinement (AMR) • Monte Carlo radiative transfer • Dust continuum • Photoionization • Atomic lines • Molecular lines • Hydrodynamics • TVD scheme with superbee flux limiter

• Self-gravity • Multigrid Poisson solver • Dirichlet boundary conditions • Lagrangian sink particles • Parallelization • Domain decomposed • MPI+openmp

Have all of the features of a dedicated radiative transfer code available for RHD calculations Haworth & Harries, 2012, MNRAS, 420, 562 Mind The Gap, Cambrige 08/07/2013 Wednesday, 10 July 13

Harries 2000

Approximations 1. Hydrogen only

1. Helium and metals

2. Monochromatic radiation

2. Polychromatic

3. The on the spot approximation

3. Diffuse field

1. Simplified thermal balance

1. Match heating/cooling rates

1. Photoionization equilibrium

1. Time dependent photoinization

Resolution?

Limited to 2D models to explore this at present Mind The Gap, Cambrige 08/07/2013

Wednesday, 10 July 13

Approximations 1. Hydrogen only

1. Helium and metals

2. Monochromatic radiation

2. Polychromatic

3. The on the spot approximation

3. Diffuse field

1. Simplified thermal balance

1. Match heating/cooling rates

1. Photoionization equilibrium

1. Time dependent photoinization

Resolution?

Limited to 2D models to explore this at present Mind The Gap, Cambrige 08/07/2013

Wednesday, 10 July 13

Models

Osterbrock – astrophysics of gaseous nebulae and AGN

Fits to Verner & Ferland 1996, ApJ, 106, 467 Mind The Gap, Cambrige 08/07/2013

Wednesday, 10 July 13

Models

Osterbrock – astrophysics of gaseous nebulae and AGN

Fits to Verner & Ferland 1996, ApJ, 106, 467 Mind The Gap, Cambrige 08/07/2013

Wednesday, 10 July 13

Initial setup 2D slab No gravity, free fall time 3Myr, tend=200kyr (not important from 3D model test) Star at centre of grid

4 Bonnor-Ebert spheres Mind The Gap, Cambrige 08/07/2013 Wednesday, 10 July 13

Pictures

Mind The Gap, Cambrige 08/07/2013 Wednesday, 10 July 13

Ionized/neutral mass

Mind The Gap, Cambrige 08/07/2013 Wednesday, 10 July 13

The density distribution

Mind The Gap, Cambrige 08/07/2013 Wednesday, 10 July 13

Summarised differences

Mind The Gap, Cambrige 08/07/2013 Wednesday, 10 July 13

Conclusions I get no resolution convergence The disruption to the density distribution seems to converge with diffuse fields, helium and metals, not too sensitive to the thermal balance. High sensitivity to the recombination coefficient used/diffuse field treatment Difficult to make quantitative conclusions using RHD models This is just one code! Keep an eye out for StarBench-2 Mind The Gap, Cambrige 08/07/2013 Wednesday, 10 July 13

Plug/Questions?

http://www.astro.ex.ac.uk/people/th2/torus_html/homepage.html Haworth & Harries, 2012, MNRAS, 420, 562 Haworth et al., 2012, MNRAS, 426, 203 Haworth et al., 2013, MNRAS, 431, 3470

Haworth et al., 2013, in prep

Mind The Gap, Cambrige 08/07/2013 Wednesday, 10 July 13

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