GTC/CanariCam mid-IR imaging of the fullerene-rich planetary nebula IC 418
The formation process(es) of fullerenes in space is still uncertain and several mechanisms have been proposed in the literature. In particular, the most accepted idea to explain the simultaneous presence of fullerenes and PAH-like emission in the H-rich circumstellar envelopes of PNe is that these molecular species may be formed from the
Díaz-Luis, J. J. et al.
Fecha de publicación:
10
2017