Herschel-Planck dust optical-depth and column-density maps : I. Method description and results for Orion

We present high-resolution, high dynamic range column-density and color-temperature maps of the Orion complex using a combination of Planck dust-emission maps, Herschel dust-emission maps, and 2MASS NIR dust-extinction maps. The column-density maps combine the robustness of the 2MASS NIR extinction maps with the resolution and coverage of the Herschel and Planck dustemission maps and constitute the highest dynamic range column-density maps ever constructed for the entire Orion complex, covering 0:01 mag < AK < 30 mag, or 2 7 1020 cm-2 < N < 5 7 1023 cm-2. We determined the ratio of the 2:2 \u3bcm extinction coefficient to the 850 \u3bcm opacity and found that the values obtained for both Orion A and B are significantly lower than the predictions of standard dust models, but agree with newer models that incorporate icy silicate-graphite conglomerates for the grain population. We show that the cloud projected probability distribution function, over a large range of column densities, can be well fitted by a simple power law. Moreover, we considered the local Schmidt-law for star formation, and confirm earlier results, showing that the protostar surface density \u3a3*follows a simple law \u3a3* 1d \u3a3\u3b2gas, with \u3b2 2. \ua9 ESO, 2014