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Infrared studies of the stellar population in Baade'S Window
Published online by Cambridge University Press: 04 August 2017
Extract
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