 Ophiuchi main cloud
  Ophiuchi main cloudA. Abergel, J.P. Bernard , F. Boulanger, C. Cesarsky, F.X. Désert, E. Falgarone, G. Lagache, M. Perault, J.-L. Puget, W.T. Reach, L. Nordh, G. Olofsson 3, M. Huldtgren, A.A. Kaas , P. André, S. Bontemps, M. Burgdorf, E. Copet, J. Davies , T. Montmerle, P. Persi, F. Sibille
We present preliminary results of the ISOCAM survey 
of the   Ophiuchi main cloud L1688 (0.5 square degrees) conducted
in the two broad-band 
filters LW2 (5-8.5
  Ophiuchi main cloud L1688 (0.5 square degrees) conducted
in the two broad-band 
filters LW2 (5-8.5   m) and LW3 (12-18
 m) and LW3 (12-18   m). This letter focuses on the
properties of the extended emission. The high angular resolution and
sensitivity of the ISOCAM observations have revealed  
several previously unknown characteristics of the mid-IR diffuse
emission: the small scale filamentary 
structure (thickness  0.03 pc) of the emission at the
illuminated edge of  
the molecular cloud, the sharpness of color variations at cloud edges, 
the barely resolved filamentary structure of the dust emission 
surrounding a bright embedded source, and several dense cores 
seen as sharp and deep absorption structures against the diffuse cloud
background.
 m). This letter focuses on the
properties of the extended emission. The high angular resolution and
sensitivity of the ISOCAM observations have revealed  
several previously unknown characteristics of the mid-IR diffuse
emission: the small scale filamentary 
structure (thickness  0.03 pc) of the emission at the
illuminated edge of  
the molecular cloud, the sharpness of color variations at cloud edges, 
the barely resolved filamentary structure of the dust emission 
surrounding a bright embedded source, and several dense cores 
seen as sharp and deep absorption structures against the diffuse cloud
background.
Keywords:
- ISM: individual objects:   Ophiuchus
- ISM: dust, extinction - ISM: clouds - Infrared: ISM: clouds
  Ophiuchus
- ISM: dust, extinction - ISM: clouds - Infrared: ISM: clouds