Abstract

New-infrared JHKL photometry is presented for a sample of 141 IRAS objects, selected on the basis of their IRAS colours and lying in two strips across the Galactic Bulge between 7°< |b| < 8° and 345°< l < 15°. Natures of the sources, and periods and bolometric magnitudes of the variables are determined. Properties of the 113 Mira stars identified in the sample are analysed.

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