Published on:
11 September 2023
Primary Category:
High Energy Astrophysical Phenomena
Paper Authors:
Kaho Tse,
Duncan K. Galloway,
Alexander Heger
Oscillations discovered in archival X-ray data from 2006-2007 outburst of XTE J1701-462
Signals occur from 3.5-5.6 millihertz frequency range
Amplitudes around 1% indicate marginally stable nuclear burning origin
First such discovery in a Z-type low mass X-ray binary
Tenth source overall found to show this rare phenomenon
Discovery of millihertz oscillations in XTE J1701-462
This paper reports the discovery of rare millihertz quasi-periodic oscillations in the low mass X-ray binary XTE J1701-462. The oscillations were found by searching archival data from NASA's Rossi X-ray Timing Explorer satellite covering the 2006-2007 outburst of the source. The oscillations occur between 3.5-5.6 millihertz, have amplitudes around 1%, and are interpreted as arising from marginally stable nuclear burning on the surface of the neutron star. This is only the tenth source found to exhibit this phenomenon, providing new insights into thermonuclear burning processes in extreme environments.
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