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Observational study identifies new dipper star candidates and long-period eclipsing binaries, suggesting new insights into variable stars.
Dipper stars are extrinsically variable stars with deep dimming events due to extended, often dusty, structures produced by a wide range of mechanisms such as collisions, protoplanetary evolution or stellar winds. ASAS-SN has discovered 12 dipper-like objects as part of its normal operations. Here we systematically search the ∼ 5.1 million ASAS-SN targets with 13 < g < 14 ~mag for dippers with Δ g ≥ 0.3 ~mag to identify 4 new candidates. We also discover 15 long-period eclipsing binary candidates. We characterized the 19 new and 12 previously discovered objects using the ASAS-SN light curves and archival multi-wavelength data. We divide them into three categories: long-period eclipsing binaries with a single eclipse (13 total), long-period eclipsing binaries with multiple eclipses (7 total) and dipper stars with dust or disk occultations (11 total).
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JoHantgen et al. (2026) studied this question.
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