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NGC 2264 IRS1: The central engine and its cavity

Katharina Schreyer·Bringfried Stecklum·Hendrik Linz·Thomas Henning
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Abstract

We present a high-resolution study of NGC 2264 IRS1 in CS(2-1) and in the 3-mm continuum using the IRAM Plateau de Bure Interferometer. We complement these radio data with images taken at 2.2, 4.6, and 11.9 micron. The combined information allow a new interpretation of the closest environment of NGC 2264 IRS1. No disk around the B-type star IRS1 was found. IRS1 and its low-mass companions are located in a low-density cavity which is surrounded by the remaining dense cloud core which has a clumpy shell-like structure. Strong evidence for induced on-going star formation was found in the surroundings of IRS1. A deeply embedded very young stellar object 20 arcsec to the north of IRS1 is powering a highly collimated bipolar outflow. The object 8 in the closer environment of IRS1 is a binary surrounded by dusty circumbinary material and powering two bipolar outflows.

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Katharina Schreyer, Bringfried Stecklum, Hendrik Linz, Thomas Henning. 2003-11-06. NGC 2264 IRS1: The central engine and its cavity. https://doi.org/10.1086/379141

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