arXiv · astro-ph/0509374
Mid-Infrared Imaging of a Young Bipolar Nebula in the S287 Molecular Cloud
Abstract
We present diffraction-limited images in the 11.3 micron PAH band and in the continuum at 11.9 microns of the S287B star forming region obtained with the newly commissioned mid-infrared imager/spectrometer VISIR at the VLT. In both filters five point-like sources are detected, of which at least one has a spectral energy distribution reminiscent of a Lada Class I source. We also report on the discovery of a new Herbig Ae star in this region. It is particularly striking that the brightest mid-infrared source in this region has not been detected at shorter wavelengths; it is a good candidate to be the driving source of the bipolar molecular outflow and optical reflection nebulosity previously reported in S287B.
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M. E. van den Ancker. 2005-09-14. Mid-Infrared Imaging of a Young Bipolar Nebula in the S287 Molecular Cloud. https://doi.org/10.1051/0004-6361%3A200500188
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