Mapping the PAHs and H2 in ρ Oph A

Abstract

We present an ISOCAM-CVF map of the Oph A region, covering 3 3. For each 6 arcsec2 pixel, we extract the spectrum from 515 m. We determine the fluxes of the main PAH features by fitting Lorentzian profiles to the spectrum. The peaks of the various PAH components correspond well with the known positions of the PDRs in this vicinity. The spectrum in several pixels exhibits strong rotational lines of molecular hydrogen which can be used to derive the physical properties of the cloud. The H2 emission traces the hot gas of the bipolar CO outflow from VLA1623. © 2008 International Astronomical Union.