Multi-wavelength carbon recombination line observations with the VLA toward an UCHII region in W48: Physical properties and kinematics of neutral material

Details Multi-wavelength carbon recombination line observations with the VLA toward an UCHII region in W48: Physical properties and kinematics of neutral material Multi-wavelength carbon recombination line observations with the VLA toward an UCHII region in W48: Physical properties and kinematics of neutral material

2005-03-03

arxiv.org/abs/astro-ph/0503063v1

Astronomy and Astrophysics

Astrophysics

25 pages, 5 figures, ApJ in Press

Scientific paper

Using the Very Large Array (VLA) the C76$\alpha$ and C53$\alpha$ recombination lines (RLs) have been detected toward the ultra-compact \HII\ region (UCHII region) G35.20$-$1.74. We also obtained upper limits to the carbon RLs at 6 cm (C110$\alpha$ & C111$\alpha$) and 3.6 cm (C92$\alpha$) wavelengths with the VLA. In addition, continuum images of the W48A complex (which includes G35.20$-$1.74) are made with angular resolutions in the range 14\arcsec to 2\arcsec. Modeling the multi-wavelength line and continuum data has provided the physical properties of the UCHII region and the photodissociation region (PDR) responsible for the carbon RL emission. The gas pressure in the PDR, estimated using the derived physical properties, is at least four times larger than that in the UCHII region. The dominance of stimulated emission of carbon RLs near 2 cm, as implied by our models, is used to study the relative motion of the PDR with respect to the molecular cloud and ionized gas. Our results from the kinematical study are consistent with a pressure-confined UCHII region with the ionizing star moving with respect to the molecular cloud. However, based on the existing data, other models to explain the extended lifetime and morphology of UCHII regions cannot be ruled out.

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