Authors: Herbert Weidner
The two stars in TZ Mensae emit gravitational waves with a frequency of 2.70 $mu$Hz, which may be measured here on Earth. The decoding of the phase modulations of the GW shows eleven companions. The orbital times of the planets fit well with the predictions of Dermott's law. The physical interpretation of the result of the phase modulation is difficult, but allows the masses of the planets to be estimated.
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[v1] 2023-08-29 10:45:11
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