Identifying Blue Large Amplitude Pulsators in the Galactic Plane using Gaia DR2: a case study

Abstract

Blue Large Amplitude Pulsators (BLAPs) are blue stars showing high amplitude (>0.2 mag) pulsations on a timescale of a few tens of mins. They form a new class of variable star recently discovered using OGLE data. It has lead to a number of investigations searching for the origin of these pulsations. This short study presents the Gaia DR2 data of ten BLAPs which have parallax measurements. We have dereddened their colours using Gaia DR2 data from the stars in their immediate field and find that six show absolute magnitude and intrinsic colour consistent with expectations, whilst four stars have a less certain classification. This work highlights the extra information which Gaia DR2 data can provide to help classify those variable stars which do not currently have moderate resolution optical spectra and make searches for BLAPs in wide field high cadence surveys more systematic and robust.

Accepted by A&A as a Letter to the Editor

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Cited by in corpus (9)

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• Shell helium-burning hot subdwarf B stars as candidates for blue large-amplitude pulsators
• Identifying Blue Large Amplitude Pulsators from Gaia DR2 & ZTF DR3
• An 18.9-minute Blue Large-Amplitude Pulsator Crossing the 'Hertzsprung Gap' of Hot Subdwarfs
• The OmegaWhite Survey for Short-Period Variable Stars VII: High amplitude, short period blue variables
• Confirmation of Monoperiodicity Above 20 Seconds for Two Blue Large-Amplitude Pulsators
• The oscillation properties of the Blue Large Amplitude Pulsators (BLAPs): relative change rate of periods, excitations, and period relations