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| Paper: |
Galactic Center Pulsars with the ngVLA |
| Monograph: |
7, Science with a Next Generation Very Large Array |
| Page: |
793 |
| Authors: |
Bower, G. C.; Chatterjee, S.; Cordes, J.; Demorest, P.; Deneva, J. S.; Dexter, J.; Kramer, M.; Lazio, J.; Ransom, S.; Shao, L.; Wex, N.; Wharton, R. |
| 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° 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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