Table 1
Overview of simulations performed.
| Run | Mcore | ρ ∝ rβ | RTM | Epoch of E ≈ 1 |
|
|
||||
| A-RT+FLD | 100 | –2 | RT+FLD | No |
| A-FLD | 100 | –2 | FLD | Yes |
| B-RT+FLD | 50 | –2 | RT+FLD | No |
| B-FLD | 50 | –2 | FLD | Yes |
| C-RT+FLD | 100 | –1.5 | RT+FLD | No |
| C-FLD | 100 | –1.5 | FLD | Yes |
Notes. The table contains the run label (Col. 1), the two distinguishing parameters of the different initial conditions, namely the initial pre-stellar core mass Mcore (Col. 2) and the exponent β of the initial density slope ρ(r) (Col. 3), in addition to the radiation transport method (RTM) in use (Col. 4), and the resulting existence of an epoch of marginal Eddington equilibrium E ≈ 1 (Col. 5).
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