Astrophysics

    

Thickenings in the Ring System of the Binary Star V4046 Sagittarii

Authors: Herbert Weidner

The protoplanetary disk orbiting textit{V4046 Sagittarii} may contain planets. The central binary system $A1-A2$ emits gravitational waves with a frequency of 9.56 $mu$Hz, which may be measured here on Earth. The decoding of the phase modulations of the GW provides evidence that there are textit{twelve} rings that are not rotationally symmetric. Some may contain young planets. The orbital times fit well with the predictions of Dermott's law. The physical interpretation of the result of the phase modulation is difficult, but allows the asymmetry of the mass distribution to be estimated.

Comments: 8 Pages.

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Submission history

[v1] 2023-08-25 16:25:18

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