Table 1
Summary of the setups of the different runs.
EOS | Rcloudlet [au] | b[au] | vinf [cm s−1 ] | Tcloudlet [K] | M*∕M⊙ | bcrit | Turb? | vbackground | |
---|---|---|---|---|---|---|---|---|---|
A1 | adia | 887 | 1774 | 1.0 | 30 | 2.5 | 2218 | No | Yes |
A2 | adia | 1330 | 1774 | 1.0 | 30 | 2.5 | 2218 | No | Yes |
A3 | adia | 2662 | 2218 | 1.0 | 30 | 2.5 | 2218 | No | yes |
I1 | iso | 887 | 1774 | 1.0 | 10 | 2.5 | 2218 | No | Yes |
I2 | iso | 1330 | 1774 | 1.0 | 10 | 2.5 | 2218 | No | Yes |
I3 | iso | 2662 | 2218 | 1.0 | 10 | 2.5 | 2218 | No | Yes |
A1_t | adia | 887 | 1774 | 1.0 | 30 | 2.5 | 2218 | Yes | Yes |
A2_t | adia | 1330 | 1774 | 1.0 | 30 | 2.5 | 2218 | Yes | Yes |
A3_t | adia | 2662 | 2218 | 1.0 | 30 | 2.5 | 2218 | Yes | Yes |
I1_t | iso | 887 | 1774 | 1.0 | 10 | 2.5 | 2218 | Yes | Yes |
I2_t | iso | 1330 | 1774 | 1.0 | 10 | 2.5 | 2218 | Yes | Yes |
I3_t | iso | 2662 | 2218 | 1.0 | 10 | 2.5 | 2218 | Yes | Yes |
A1_t_nw | adia | 887 | 1774 | 1.0 | 30 | 2.5 | 2218 | Yes | No |
A2_t_nw | adia | 1330 | 1774 | 1.0 | 30 | 2.5 | 2218 | Yes | No |
A3_t_nw | adia | 2662 | 2218 | 1.0 | 30 | 2.5 | 2218 | Yes | No |
I1_t_nw | iso | 887 | 1774 | 1.0 | 10 | 2.5 | 2218 | Yes | No |
I2_t_nw | iso | 1330 | 1774 | 1.0 | 10 | 2.5 | 2218 | Yes | No |
I3_t_nw | iso | 2662 | 2218 | 1.0 | 10 | 2.5 | 2218 | Yes | No |
IrrI1_t | Tirr(r) | 887 | 1774 | 1.0 | 10 | 2.5 | 2218 | Yes | Yes |
IrrI2_t | Tirr(r) | 1330 | 1774 | 1.0 | 10 | 2.5 | 2218 | Yes | Yes |
IrrI3_t | Tirr(r) | 2662 | 2218 | 1.0 | 10 | 2.5 | 2218 | Yes | Yes |
IrrI1_t0 | Tirr(r) | 887 | 0 | 1.0 | 10 | 2.5 | 2218 | Yes | Yes |
IrrI1_t500 | Tirr(r) | 887 | 500 | 1.0 | 10 | 2.5 | 2218 | Yes | Yes |
IrrI1_t1000 | Tirr(r) | 887 | 1000 | 1.0 | 10 | 2.5 | 2218 | Yes | Yes |
Notes. First column: label of the individual run; second column: thermal prescription; “adia” stands for adiabatic, “iso” for isothermal, and Tirr (r) for stellar irradiation. Third column: initial cloudlet radius Rcloudlet in au; fourth column: impact parameter b in au; fifth column: initial bulk velocity of the cloudlet vinf in cm s−1 ; sixth column: initial temperature of the cloudlet Tcloudlet in K; seventh column: stellar mass in solar mass M⊙; eighth column: critical impact parameter bcrit for which the deflection angle is π∕2; ninth column: “yes” and “no” indicate whether the turbulence description is used for the initialization of the cloudlet; tenth column: “yes” and “no” indicate whether the background gas has the same initial velocity as the cloudlet (“yes”) or whether it is at rest with respect to the star (“no”).
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