... | ... | @@ -12,6 +12,8 @@ The external radiation field might be the most important heating source for grai |
|
|
1000 mum 13.2 %
|
|
|
3000 mum 10 %
|
|
|
|
|
|
|
|
|
|
|
|
**Effect of the background interstellar radiation field on the SED**
|
|
|
|
|
|
We included a uniform external radiation field to account for the heating from outside of the envelope. The protostar only heats the inner ~1000 au. If the external radiation is neglected then at few 1000 au from the central source the dust temperature might drop significantly below 10 K.
|
... | ... | |