Abstract
An IR-scan of the Baade’s Window (1 ≃ 0°.0, b ≃ −4°.0 ) area (BW) has been obtained (Ruelas-Mayorga et al., 1983). The Cumulative Counts Function (CCF) at 2.2 μm (No. of sources per sq. degree down to a given K magnitude) down to K ≃ +13.5 was formed by combining 1.9−m telescope scans with Anglo Australian Telescope (AAT) scans.
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References
Jones, T.J., Ashley, M., Hyland, A.R. and Ruelas-Mayorga, R.A.: 1981, M.N.R.A.S. 197, p. 413
Ruelas-Mayorga, R.A., Hyland, A.R. and Jones, T.J.: 1983, Ap.J. (submitted)
van den Bergh, S.: 1971, Astron. J. 76, p. 1082
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© 1985 IAU
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Ruelas-Mayorga, R.A., Hyland, A.R., Jones, T.J. (1985). Infrared Studies of the Stellar Population in Baade’s Window. In: Van Woerden, H., Allen, R.J., Burton, W.B. (eds) The Milky Way Galaxy. International Astronomical Union, vol 106. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5291-1_17
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DOI: https://doi.org/10.1007/978-94-009-5291-1_17
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