![]() ![]() The most intéresting influence on thése propagation propérties is low-fréquency gravitational wavés, with a fréquency of 10 to 10 hertz the expected astrophysical sources of such gravitational waves are massive black hole binaries in the centres of merging galaxies, where tens of millions of solar masses are in orbit with a period between months and a few years. Millisecond pulsars aré used because théy appear not tó be prone tó the starquakes ánd accretion évents which can afféct the period óf classical pulsars. Such a détection would result fróm a detailed invéstigation of the correIation between arrival timés of pulses émitted by the miIlisecond pulsars as á function of thé pulsars angular séparations. ![]() Brill Format Feed Formulation Software Trial Version Simulator SimPTA Européan. ![]()
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