Figure 1 Evolution of the FUV flux in

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Figure 1. Evolution of the FUV flux in one simulated star-forming region where the

Figure 1. Evolution of the FUV flux in one simulated star-forming region where the initial local stellar density is. . . Mon Not R Astron Soc, Volume 502, Issue 2, April 2021, Pages 2665– 2681, https: //doi. org/10. 1093/mnras/stab 054 The content of this slide may be subject to copyright: please see the slide notes for details.

Figure 2. The effect of varying the initial local stellar density (the volume density

Figure 2. The effect of varying the initial local stellar density (the volume density within a sphere that encompasses. . . Mon Not R Astron Soc, Volume 502, Issue 2, April 2021, Pages 2665– 2681, https: //doi. org/10. 1093/mnras/stab 054 The content of this slide may be subject to copyright: please see the slide notes for details.

Figure 3. Comparison of the evolution of star-forming regions with different fractal dimensions but

Figure 3. Comparison of the evolution of star-forming regions with different fractal dimensions but with constant. . . Mon Not R Astron Soc, Volume 502, Issue 2, April 2021, Pages 2665– 2681, https: //doi. org/10. 1093/mnras/stab 054 The content of this slide may be subject to copyright: please see the slide notes for details.

Figure 4. The effect of varying the initial virial ratios when the initial stellar

Figure 4. The effect of varying the initial virial ratios when the initial stellar density is kept constant. . . Mon Not R Astron Soc, Volume 502, Issue 2, April 2021, Pages 2665– 2681, https: //doi. org/10. 1093/mnras/stab 054 The content of this slide may be subject to copyright: please see the slide notes for details.

Figure 5. Comparison of different mass distributions with constant initial stellar density ($tilde{rho }

Figure 5. Comparison of different mass distributions with constant initial stellar density ($tilde{rho } sim. . . Mon Not R Astron Soc, Volume 502, Issue 2, April 2021, Pages 2665– 2681, https: //doi. org/10. 1093/mnras/stab 054 The content of this slide may be subject to copyright: please see the slide notes for details.

Figure 6. The evolution of discs in our default simulation ($tilde{rho } sim 100$

Figure 6. The evolution of discs in our default simulation ($tilde{rho } sim 100$ M⊙ pc− 3, D =. . . Mon Not R Astron Soc, Volume 502, Issue 2, April 2021, Pages 2665– 2681, https: //doi. org/10. 1093/mnras/stab 054 The content of this slide may be subject to copyright: please see the slide notes for details.

Figure A 1. Evolution of a single disc in a radiation field where the

Figure A 1. Evolution of a single disc in a radiation field where the disc radius is allowed to evolve according to. . . Mon Not R Astron Soc, Volume 502, Issue 2, April 2021, Pages 2665– 2681, https: //doi. org/10. 1093/mnras/stab 054 The content of this slide may be subject to copyright: please see the slide notes for details.

Figure A 2. Evolution of a single disc in a radiation field where the

Figure A 2. Evolution of a single disc in a radiation field where the disc radius is allowed to evolve according to. . . Mon Not R Astron Soc, Volume 502, Issue 2, April 2021, Pages 2665– 2681, https: //doi. org/10. 1093/mnras/stab 054 The content of this slide may be subject to copyright: please see the slide notes for details.

Figure A 3. Evolution of a single disc in a radiation field where the

Figure A 3. Evolution of a single disc in a radiation field where the disc radius is allowed to evolve according to. . . Mon Not R Astron Soc, Volume 502, Issue 2, April 2021, Pages 2665– 2681, https: //doi. org/10. 1093/mnras/stab 054 The content of this slide may be subject to copyright: please see the slide notes for details.

Figure A 4. Evolution of a single disc in a radiation field where the

Figure A 4. Evolution of a single disc in a radiation field where the disc radius is allowed to evolve according to. . . Mon Not R Astron Soc, Volume 502, Issue 2, April 2021, Pages 2665– 2681, https: //doi. org/10. 1093/mnras/stab 054 The content of this slide may be subject to copyright: please see the slide notes for details.

Figure A 5. Evolution of a single disc in a radiation field where the

Figure A 5. Evolution of a single disc in a radiation field where the disc radius is allowed to evolve according to. . . Mon Not R Astron Soc, Volume 502, Issue 2, April 2021, Pages 2665– 2681, https: //doi. org/10. 1093/mnras/stab 054 The content of this slide may be subject to copyright: please see the slide notes for details.

Figure B 1. Comparison of the evolution of disc fractions in our default simulation

Figure B 1. Comparison of the evolution of disc fractions in our default simulation ($tilde{rho } =. . . Mon Not R Astron Soc, Volume 502, Issue 2, April 2021, Pages 2665– 2681, https: //doi. org/10. 1093/mnras/stab 054 The content of this slide may be subject to copyright: please see the slide notes for details.