Astrophysics

    

Detection of the Continuous Gravitational Wave of HM Cancri

Authors: Herbert Weidner

HM Cancri is expected to be be one of the brightest sources of gravitational waves in our galaxy. Despite its known frequency, the radiation could not be detected so far. A novel technique can compensate for phase modulation and detect this GW in the records of superconducting gravimeters. This new observational window will allow a deeper understanding of the enigmatic stellar system.

Comments: 12 Pages.

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Submission history

[v1] 2022-01-25 09:39:44
[v2] 2022-06-26 13:41:33

Unique-IP document downloads: 336 times

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