A Catalog of Background Stars Reddened by Dust in the Taurus Dark Clouds
arXiv:0801.4050 · doi:10.1086/533532
Abstract
Normal field stars located behind dense clouds are a valuable resource in interstellar astrophysics, as they provide continua in which to study phenomena such as gas-phase and solid-state absorption features, interstellar extinction and polarization. This paper reports the results of a search for highly reddened stars behind the Taurus Dark Cloud complex. We use the Two Micron All Sky Survey (2MASS) Point Source Catalog to survey a 50 sq deg area of the cloud to a limiting magnitude of K = 10.0. Photometry in the 1.2-2.2 micron passbands from 2MASS is combined with photometry at longer infrared wavelengths (3.6-12 micron) from the Spitzer Space Telescope and the Infrared Astronomical Satellite to provide effective discrimination between reddened field stars and young stellar objects (YSOs) embedded in the cloud. Our final catalog contains 248 confirmed or probable background field stars, together with estimates of their total visual extinctions, which span the range 2-29 mag. We also identify the 2MASS source J04292083+2742074 (IRAS 04262+2735) as a previously unrecognized candidate YSO, based on the presence of infrared emission greatly in excess of that predicted for a normal reddened photosphere at wavelengths >5 microns.
References in corpus (5)
- The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)
- The Efficiency of Grain Alignment in Dense Interstellar Clouds: A Reassessment of Constraints from Near Infrared Polarization
- A Survey for New Members of Taurus with the Spitzer Space Telescope
- Coronal abundances of X-ray bright pre-main sequence stars in the Taurus Molecular Cloud
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Cited by in corpus (5)
- The relation between gas and dust in the Taurus Molecular Cloud
- Probing Interstellar Grain Growth Through Polarimetry in the Taurus Cloud Complex
- Study of magnetic field geometry and extinction in Bok globule CB130
- Chemical and Physical Conditions in Molecular Cloud Core DC 000.4-19.5 (SL42) in Corona Australis
- An Improved Pair Method to Probe the Dust Extinction Law