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101 results on '"Bullock, James"'

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3. What Causes The Formation of Disks and End of Bursty Star Formation?

5. FIREbox: Simulating galaxies at high dynamic range in a cosmological volume

7. FIRE-3: updated stellar evolution models, yields, and microphysics and fitting functions for applications in galaxy simulations

9. Star formation at the edge of the Local Group: a rising star formation history in the isolated galaxy WLM

10. Hot-mode accretion and the physics of thin-disc galaxy formation

14. The galaxy–halo size relation of low-mass galaxies in FIRE

16. Star formation at the edge of the Local Group: a rising star formation history in the isolated galaxy WLM

17. The bursty origin of the Milky Way thick disc

21. The time-scales probed by star formation rate indicators for realistic, bursty star formation histories from the FIRE simulations

22. Spatially resolved star formation and fuelling in galaxy interactions

23. A dark matter profile to model diverse feedback-induced core sizes of ΛCDM haloes

25. Stars made in outflows may populate the stellar halo of the Milky Way

26. A profile in FIRE: resolving the radial distributions of satellite galaxies in the Local Group with simulations

27. Star formation at the edge of the Local Group: a rising star formation history in the isolated galaxy WLM

29. A predicted correlation between age gradient and star formation history in FIRE dwarf galaxies

30. Dwarf galaxies in CDM, WDM, and SIDM: disentangling baryons and dark matter physics

31. Star formation histories of dwarf galaxies in the FIRE simulations: dependence on mass and Local Group environment

34. The total dispersal kernel: a review and future directions

35. Advancing an interdisciplinary framework to study seed dispersal ecology

36. The haloes and environments of nearby galaxies (HERON) – I. Imaging, sample characteristics, and envelope diameters

39. The Local Group on FIRE: dwarf galaxy populations across a suite of hydrodynamic simulations

40. Employing plant functional groups to advance seed dispersal ecology and conservation

43. The origin of the diverse morphologies and kinematics of Milky Way-mass galaxies in the FIRE-2 simulations

46. FIRE-2 simulations: physics versus numerics in galaxy formation

47. No assembly required: mergers are mostly irrelevant for the growth of low-mass dwarf galaxies

49. Dwarf galaxy mass estimators versus cosmological simulations

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