Protostellar Outflow Heating in a Growing Massive Protocluster
arXiv:1112.1885 · doi:10.1088/2041-8205/745/2/L30
Abstract
The dense molecular clump P1 in the infrared dark cloud (IRDC) complex G28.34+0.06 harbors a massive protostellar cluster at its extreme youth. Our previous Submillimeter Array (SMA) observations revealed several jet-like CO outflows emanating from the protostars, indicative of intense accretion and potential interaction with ambient natal materials. Here we present the Expanded Very Large Array (EVLA) spectral line observations toward P1 in the NH3 (J,K) = (1,1), (2,2), (3,3) lines, as well as H2O and class I CH3OH masers. Multiple NH3 transitions reveal the heated gas widely spread in the 1 pc clump. The temperature distribution is highly structured; the heated gas is offset from the protostars, and morphologically matches the outflows very well. Hot spots of spatially compact, spectrally broad NH3 (3,3) emission are also found coincident with the outflows. A weak NH3 (3,3) maser is discovered at the interface between an outflow jet and the ambient gas. These findings suggest that protostellar heating may not be effective in suppressing fragmentation during the formation of massive cores.
15 pages, 4 figures, 1 table, accepted to ApJ Letters
References in corpus (11)
- Magnetically Regulated Star Formation in 3D: The Case of Taurus Molecular Cloud Complex
- The effect of magnetic fields on star cluster formation
- Hierarchical Fragmentation and Jet-like Outflows in IRDC G28.34+0.06, a Growing Massive Protostar Cluster
- A submillimetre survey of the kinematics of the Perseus molecular cloud - II. Molecular outflows
- Radiation Feedback and Fragmentation in Massive Protostellar Cores
- NH3 Observations of the Infrared Dark Cloud G28.34+0.06
- Very Large Array Observations of Ammonia in Infrared-Dark Clouds I: Column Density and Temperature Structure
- Is protostellar heating sufficient to halt fragmentation? A case study of the massive protocluster G8.68-0.37
- Hot ammonia in NGC6334I & I(N)
- A Jet-like Outflow toward the High-Mass (Proto)stellar Object IRAS 18566+0408
- Evidence for Dynamically Important Magnetic Fields in Molecular Clouds
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- The SOFIA Massive (SOMA) Star Formation Survey. I. Overview and First Results
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- Mid-J CO shock tracing observations of infrared dark clouds II Low-J CO constraints on excitation, depletion, and kinematics
- A global view on star formation: The GLOSTAR Galactic plane survey. IX. Radio Source Catalog III: 2<l<28, 36<l<40, 56<l<60 and |b|<1, VLA B-configuration
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