Infrared excess in semi-regular variables in the Magellanic Clouds
1 Koninklijke Sterrenwacht van België (KSB), Ringlaan 3, B-1180 Brussels, Belgium
2 Astronomical Observatory of Belgrade (AOB), Volgina 7, 11 060 Belgrade, Serbia
3 Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Hungarian Academy of Sciences, H-1121 Budapest, Konkoly Thege Miklós út 15-17, Hungary
Published online: 8 September 2017
Following up on our recent work we are investigating if Type II Cepheids could be “hiding” in the sample of stars classified by the OGLE team as long-period variables.
© The Authors, published by EDP Sciences, 2017
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