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Galactic Center Pulsars with the ngVLA

Geoffrey C. Bower, Shami Chatterjee, Jim Cordes, Paul B. Demorest, J. S. Deneva, Jason Dexter, M. Krämer, Joseph Lazio, S. M. Ransom, Lijing Shao · 2018 · astro-ph.HE · DOI 10.48550/arxiv.1810.06623 · arXiv 1810.06623

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abstract

Pulsars in the Galactic Center (GC) are important probes of General Relativity, star formation, stellar dynamics, stellar evolution, and the interstellar medium. Despite years of searching, only a handful of pulsars in the central 0.5 deg are known. The high-frequency sensitivity of ngVLA will open a new window for discovery and characterization of pulsars in the GC. A pulsar in orbit around the GC black hole, Sgr A*, will provide an unprecedented probe of black hole physics and General Relativity.

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astro-ph.HE 1

years

2026 1

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ACCEPT 1

representative citing papers

Galactic Centre Pulsars with the SKAO

astro-ph.HE · 2026-07-03 · accept · novelty 4.0

Updated SKA-MID sensitivity and multi-beam search strategies can detect up to ~84% of Galactic Centre pulsars (and ~60% of MSPs) under magnetar-like scattering, unlocking precision tests around Sgr A*.

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  • Galactic Centre Pulsars with the SKAO astro-ph.HE · 2026-07-03 · accept · none · ref 146 · internal anchor

    Updated SKA-MID sensitivity and multi-beam search strategies can detect up to ~84% of Galactic Centre pulsars (and ~60% of MSPs) under magnetar-like scattering, unlocking precision tests around Sgr A*.