Polycyclic Aromatic Hydrocarbon Emission in the Proplyd HST10: What is the Mechanism behind Photoevaporation?

S. Vicente , O. Berne (1) , A. G. G. M. Tielens , N. Huélamo (2) , E. Pantin (3) , I. Kamp (4) , A. Carmona

1 CESR - Centre d'étude spatiale des rayonnements
2 CAB - Centro de Astrobiologia [Madrid]
3 ARENA - Antarctic Research a European Network for Astrophysics
4 Kapteyn Astronomical Institute [Groningen]

Mots clés: circumstellar matter; ISM: lines and bands; ISM: molecules; protoplanetary disks; stars: individual: HST10; Astrophysics - Solar and Stellar Astrophysics; Astrophysics - Astrophysics of Galaxies

Domaines: Astrophysique [astro-ph]

S. Vicente, O. Berne, A. G. G. M. Tielens, N. Huélamo, E. Pantin, et al.. Polycyclic Aromatic Hydrocarbon Emission in the Proplyd HST10: What is the Mechanism behind Photoevaporation?. apjl, 2013, 765 (2), pp.L38. ⟨10.1088/2041-8205/765/2/L38⟩. ⟨hal-02357115⟩