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- W3103300976 abstract "Radio pulsars in relativistic binary systems are unique tools to study the curved space-time around massive compact objects. The discovery of a pulsar closely orbiting the super-massive black hole at the centre of our Galaxy, Sgr A*, would provide a superb test-bed for gravitational physics. To date, the absence of any radio pulsar discoveries within a few arc minutes of Sgr A* has been explained by one principal factor: extreme scattering of radio waves caused by inhomogeneities in the ionized component of the interstellar medium in the central 100 pc around Sgr A*. Scattering, which causes temporal broadening of pulses, can only be mitigated by observing at higher frequencies. Here we describe recent searches of the Galactic centre region performed at a frequency of 18.95 GHz with the Effelsberg radio telescope." @default.
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- W3103300976 date "2012-08-01" @default.
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- W3103300976 title "Can we see pulsars around Sgr A⋆? The latest searches with the Effelsberg telescope." @default.
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- W3103300976 doi "https://doi.org/10.1017/s1743921312024209" @default.
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