2006ApJ...648..504C -
Astrophys. J., 648, 504-509 (2006/September-1)
Millimeter imaging of the HH 270 protostellar core and outflow.
CHOI M. and TANG Y.-W.
Abstract (from CDS):
The HH 270 region was observed in the C18O and the 13 CO J=1⟶0 lines with angular resolutions ranging from 3" to 10". The dense molecular core containing the centimeter continuum source VLA 1 has a mass of ∼1.6 M☉. As the 13CO image shows that the dense core is elongated in the direction perpendicular to the outflow axis, the core may be flattened and viewed nearly edge-on. The 13CO spectrum shows a blue-skewed line profile when the imaging is done at a high resolution, suggesting that the infall motion becomes kinematically important on a small scale, within ∼2000 AU from the center. The molecular outflow does not show a large line width, and the outflow axis may be close to the plane of the sky. Archival near-IR images reveal that there is a nebulosity associated with VLA 1, and that VLA 1 and HH 270 IRS are separate objects. Comparison of the near-IR and optical images with an accurate positional alignment shows that VLA 1 is the driving source of the HH 270 flow. If HH 270 IRS is not a background star, the HH 270 core may contain a binary system with inhomogeneous spectral classes: VLA 1 may be a Class 0 protostar, and HH 270 IRS may be a young stellar object with a hotter spectral energy distribution.
Abstract Copyright:
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Journal keyword(s):
ISM: Individual: Alphanumeric: HH 270 - ISM: Jets and Outflows - Stars: Formation
Simbad objects:
18
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