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Infrared studies of the stellar population in Baade'S Window

Published online by Cambridge University Press:  04 August 2017

R.A. Ruelas-Mayorga ,
A. R. Hyland  and
T. J. Jones
R.A. Ruelas-Mayorga
Affiliation:
Mount Stromlo and Siding Spring Observatories The Australian National University
A. R. Hyland
Affiliation:
Mount Stromlo and Siding Spring Observatories The Australian National University
T. J. Jones
Affiliation:
University of Minnesota

Extract

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An IR-scan of the Baade's Window () area (BW) has been obtained (Ruelas-Mayorga etal., 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.

Type
PART II: COMPOSITION, STRUCTURE AND KINEMATICS
Information
Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 129 - 130
Copyright
Copyright © Reidel 1985 

References

Jones, T.J., Ashley, M., Hyland, A.R. and Ruelas-Mayorga, R.A.: 1981, M.N.R.A.S. 197, p. 413 CrossRefGoogle Scholar
Ruelas-Mayorga, R.A., Hyland, A.R. and Jones, T.J.: 1983, Ap. J. (submitted) Google Scholar
van den Bergh, S.: 1971, Astron. J. 76, p. 1082 Google Scholar