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Aql X-1 from dawn ’til dusk: the early rise, fast state transition, and decay of its 2024 outburst

Transient low-mass X-ray binaries (LMXBs) are usually first detected by all-sky X-ray monitors when they enter new outbursts. These detections typically occur at X-ray luminosities above ∼1036 erg/s. Observations of these sources during the early rise of the outbursts have therefore been very limite...

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Hoofdauteurs: Marino A., Coti Zelati F., Alabarta K., Russell D. M., Cavecchi Y., Rea N., Rout S. K., Di Salvo T., Homan J., Jurado-López Á., Ji L., Soria R., Russell T. D., Wang Y. L., Anitra A., Baglio M. C., Feng H., Fijma S., Guillot S., Huang Y. F., Illiano G., Imbrogno M., Jin C., Lewis F., Liang Y. F., Liu M. J., Ma R., Mastroserio G., Motta S. E., Ness J. U., Parent E., Patruno A., Saikia P., Tao L., Veresvarska M., Xu X. P., Yuan W., Zhang G. B., Zhang Z. J.
Formaat: Artigo
Taal:Inglês
Gepubliceerd in: EDP Sciences 2026-06-01
Reeks:Astronomy & Astrophysics
Onderwerpen:
accretion
accretion disks
stars: neutron
x-rays: binaries
x-rays: individuals: aql x-1
Online toegang:https://www.aanda.org/articles/aa/full_html/2026/06/aa58183-25/aa58183-25.html
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