Abstract
Thanks to technological developments of detector arrays, it has been possible recently to built cameras dedicated to observations in the 10 μm atmospheric window. With these cameras, it is now easy to have access to the full angular resolution capability of 3 m class telescopes: 0.7 arcsec (the diffraction limit).
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Dent, W.: 1988, Astrophys. J. 325, 252
Dent, W., Sandell, G., Duncan, W., Robson, E.: 1989, M.N.R.A.S. 238, 1497
Lagage, P.O.: 1989, in J.P. Swings, ed(s)., “New Technologies for Astronomy”, published by SPIE, 1130, 169
Lagage, P.O.: 1992, in preparation
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© 1993 Springer Science+Business Media Dordrecht
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Lagage, P.O., Cesarski, C., Jouan, R., Masse, P., Tarrius, A., Cabrit, S. (1993). Subarcsec 10 μm Imaging of Bipolar Flow Sources. In: Errico, L., Vittone, A.A. (eds) Stellar Jets and Bipolar Outflows. Astrophysics and Space Science Library, vol 186. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1924-5_17
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DOI: https://doi.org/10.1007/978-94-011-1924-5_17
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-4851-4
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