Deep Near-Infrared Observations and Identifications of Chandra Sources in the Orion Molecular Cloud 2 and 3
arXiv:astro-ph/0211521 · doi:10.1086/346277
Abstract
We conducted deep NIR imaging observations of the Orion molecular cloud 2 and 3 using QUIRC on the 88-inch telescope of the University of Hawaii. Our purposes are 1) to generate a comprehensive NIR source catalog of these star forming clouds, and 2) to identify the NIR counterpart of the Chandra X-ray sources that have no counterpart in the 2MASS catalog. Our J-, H-, and K-band observations are about 2 mag deeper than those of 2MASS, and well match the current Chandra observation. We detected 1448 NIR sources, for which we derived the position, the J-, H-, and K-band magnitude, and the 2MASS counterpart. Using this catalog, we identified the NIR counterpart for about 42% of the 2MASS-unIDed Chandra sources. The nature of these Chandra sources are discussed using their NIR colors and spatial distributions, and a dozen protostar and brown dwarf candidates are identified.
arXiv comment39 pages, 9 postscript figures, accepted for publication in AJ
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- Infrared Nebulae Around Young Stellar Objects
- Determining the recurrence timescale of long-lasting YSO outbursts
- Discovery of Extremely Embedded X-ray Sources in the R Coronae Australis Star Forming Core
- The Gould's Belt Very Large Array Survey III. The Orion region
- Star Formation Under the Outflow: The Discovery of a Non-Thermal Jet from OMC-2 FIR 3 and its Relationship to the Deeply Embedded FIR 4 Protostar
- A High-Resolution Very Large Array Observation of a Protostar in OMC-3: Shock-induced X-ray Emission by a Protostellar Jet
- Gas velocity structure of the Orion A Integral Shaped Filament
- On the nature of the deeply embedded protostar OMC-2 FIR 4
- The JCMT Transient Survey: An Extraordinary Submillimetre Flare in the T Tauri Binary System JW 566