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The innermost jet in the hidden ultra-luminous X-ray source Cygnus X-3 · 2025 · DOI 10.1093/mnrasl/slad111

2 Pith papers cite this work. Polarity classification is still indexing.

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astro-ph.HE 2

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2026 2

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Polarimetry of Ultraluminous X-ray sources

astro-ph.HE · 2026-06-26 · unverdicted · novelty 4.0

Feasibility calculations show SKA-Mid can detect polarized emission from a Holmberg II X-1-like ULX jet within 10 hours up to ~10 Mpc, while the bubble requires ~100 hours.

Accreting Compact Object Binaries with the SKA

astro-ph.HE · 2026-06-24 · unverdicted · novelty 2.0

This perspective paper outlines expected advances in studying accretion and jets in compact object binaries using the SKA's improved sensitivity and resolution.

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Showing 2 of 2 citing papers after filters.

  • Polarimetry of Ultraluminous X-ray sources astro-ph.HE · 2026-06-26 · unverdicted · none · ref 19

    Feasibility calculations show SKA-Mid can detect polarized emission from a Holmberg II X-1-like ULX jet within 10 hours up to ~10 Mpc, while the bubble requires ~100 hours.

  • Accreting Compact Object Binaries with the SKA astro-ph.HE · 2026-06-24 · unverdicted · none · ref 77

    This perspective paper outlines expected advances in studying accretion and jets in compact object binaries using the SKA's improved sensitivity and resolution.