Abstract
Dense cores in dark clouds with obscured young stellar objects in them (showing up as IRAS sources) are excellent targets for near-infrared imaging with the new 2-dimensional infrared arrays such as IRCAM at UKIRT (58 × 62 pixels, 0.6 arcsec/pixel). Here we report some of the first results with this instrument obtained for embedded sources in the Taurus and Ophiuchus clouds (L1489, L1495; Elias 21, Elias 22). We also discuss the promise of future observations.
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Zinnecker, H. (1988). Near-Infrared Array Images of Low-Luminosity IRAS Sources in Dark Clouds. In: Dupree, A.K., Lago, M.T.V.T. (eds) Formation and Evolution of Low Mass Stars. NATO ASI Series, vol 241. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3037-7_6
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DOI: https://doi.org/10.1007/978-94-009-3037-7_6
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