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Abstract ZTF J213056.71+442046.5 is the prototype of a small class of recently discovered compact binaries composed of a white dwarf and a hot subdwarf that fills its Roche lobe. Its orbital period of only 39 minutes is the shortest known for the objects in this class. Evidence for a high orbital inclination ( i = 86°) and for the presence of an accretion disk has been inferred from a detailed modeling of its optical photometric and spectroscopic data. We report the results of an XMM-Newton observation carried out on 2021 January 7. ZTF J213056.71+442046.5 was clearly detected by the Optical Monitor, which showed a periodic variability in the UV band (200–400 nm), with a light curve similar to that seen at longer wavelengths. Despite accretion on the white dwarf at an estimated rate of the order of 10 −9 M ⊙ yr −1 , no X-rays were detected with the EPIC instrument, with a limit of ∼10 30 erg s −1 on the 0.2–12 keV luminosity. We discuss possible explanations for the lack of a strong X-ray emission from this system.more » « less
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Acero, F. ; Acharyya, A. ; Adam, R. ; Aguasca-Cabot, A. ; Agudo, I. ; Aguirre-Santaella, A. ; Alfaro, J. ; Aloisio, R. ; Crespo, N. Álvarez ; Batista, R. Alves ; et al ( , Astroparticle Physics)Free, publicly-accessible full text available August 1, 2024
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Adams, C.B. ; Alfaro, R. ; Ambrosi, G. ; Ambrosio, M. ; Aramo, C. ; Arlen, T. ; Batista, P.I. ; Benbow, W. ; Bertucci, B. ; Bissaldi, E. ; et al ( , Astroparticle Physics)null (Ed.)