Volume 536, December 2011
|Number of page(s)||18|
|Section||Interstellar and circumstellar matter|
|Published online||06 December 2011|
Mass reservoirs surrounding massive infrared dark clouds
A view by near-infrared dust extinction⋆
Max-Planck-Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
e-mail: email@example.com; firstname.lastname@example.org; email@example.com
2 Institute for Astronomy, University of Vienna, Türkenschanzstrasse 17, 1180 Vienna, Austria
3 Max-Planck-Institutfür Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
Received: 23 July 2011
Accepted: 26 September 2011
Context. Infrared dark clouds (IRDCs) harbor progenitors of high-mass stars. Little is known of the parental molecular clouds of IRDCs.
Aims. We demonstrate the feasibility of the near-infrared (NIR) dust extinction mapping in tracing the parental molecular clouds of IRDCs at the distances of D ≈ 2.5−8 kpc.
Methods. We derive NIR extinction maps for 10 prominent IRDC complexes using a color-excess mapping technique and NIR data from the UKIDSS/Galactic Plane Survey. We compare the resulting maps to the 13CO emission line data, to the 8 μm dust opacity data, and to the millimeter dust emission data. We derive distances for the clouds by comparing the observed NIR source densities to the Besançon stellar distribution model and compare them to the kinematic distance estimates.
Results. The NIR extinction maps provide a view of the IRDC complexes over the dynamical range of AV ≈ 2 − 40 mag, in spatial resolution of ~30″. The NIR extinction data correlate well with the 13CO data and probe a similar gas component, but also extend to higher column densities. The NIR data reveal a wealth of extended structures surrounding the dense gas traced by the 8 μm shadowing features and sub-mm dust emission, showing that the clouds contain typically ≳ 10 times more mass than traced by those tracers. The IRDC complexes of our sample contain a relatively high amount of high-column density material, and their cumulative column density distributions resemble active nearby star-forming clouds like Orion rather than less active clouds like California.
Conclusions. The NIR dust extinction data provide a new powerful tool to probe the mass distribution of the parental molecular clouds of IRDCs up to the distances of D ~ 8 kpc. This encourages deeper NIR observations of IRDCs, because the sensitivity and resolution of the data can be directly enhanced with dedicated observations. In addition to mass distributions, the NIR data provide relatively reliable distance estimates.
Key words: ISM: clouds / evolution / ISM: structure / dust, extinction
Appendix A is available in electronic form at http://www.aanda.org
© ESO, 2011
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