Volume 499, Number 1, May III 2009
|Page(s)||175 - 189|
|Section||Interstellar and circumstellar matter|
|Published online||18 February 2009|
Mapping outflows in the collapsing protocluster NGC 2264-C
Laboratoire AIM, CEA/DSM-CNRS-Université Paris Diderot, IRFU/Service d'Astrophysique, C.E. Saclay, Orme des Merisiers, 91191 Gif-sur-Yvette, France
2 Department of Astronomy, University of Virginia, PO Box 400325, Charlottesville, VA 22904, USA
Accepted: 6 February 2009
Context. The role played by protostellar feedback in clustered star formation is still a matter of debate. In particular, protostellar outflows have been proposed as a source of turbulence in cluster-forming clumps, which may provide support against global collapse for several free-fall times.
Aims. Here, we seek to test the above hypothesis in the case of the well-documented NGC 2264-C protocluster, by quantifying the amount of turbulence and support injected in the surrounding medium by protostellar outflows.
Methods. Using the HERA heterodyne array on the IRAM 30 m telescope, we carried out an extensive mapping of NGC 2264-C in the three molecular line transitions 12CO(2–1), 13CO(2–1), and C18O(2–1).
Results. We found widespread high-velocity 12CO emission, testifying to the presence of eleven outflow lobes, closely linked to the compact millimeter continuum sources previously detected in the protocluster. We carried out a detailed analysis of the dynamical parameters of these outflows, including a quantitative evaluation of the overall momentum flux injected in the cluster-forming clump. These dynamical parameters were compared to the gravitational and turbulent properties of the clump.
Conclusions. We show that the population of protostellar outflows identified in NGC 2264-C is likely to contribute a significant fraction of the observed turbulence but cannot efficiently support the protocluster against global collapse. Gravity appears to largely dominate the dynamics of the NGC 2264-C clump at the present time; however it is possible that an increase in the star formation rate during the later evolution of the protocluster will trigger enough outflows to finally halt the contraction of the cloud.
Key words: stars: formation / stars: circumstellar matter / ISM: clouds / ISM: structure / ISM: jets and outflows / ISM : individual objects: NGC 2264-C
Based on observations carried out with the IRAM 30 m telescope. IRAM is supported by INSU/CNRS (France), MPG (Germany), and IGN (Spain).
© ESO, 2009
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