Michael E. Ressler, M. Barsony
Abstract
WL16 is unique among the members of the young, forming star cluster embedded in the nearby p Oph cloud core in exhibiting an extended, high surface brightness disk in the emission features originating from solid-state aromatic hydrocarbons.
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WL16 is unique among the members of the young, forming star cluster embedded in the nearby p Oph cloud core in exhibiting an extended, high surface brightness disk in the emission features originating from solid-state aromatic hydrocarbons.
Key concepts: Physics, Astrophysics, Surface brightness, Young stellar object, Star formation, Infrared, Astronomy, Brightness