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arXiv · 2202.04949

A Hot Subdwarf Model for the 18.18 Minute Pulsar GLEAM-X

Abraham Loeb·Dan Maoz
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Abstract

We suggest that the recently discovered, enigmatic pulsar with a period of 18.18 minutes, GLEAM-X J162759.5-523504.3, is most likely a hot subdwarf (proto white dwarf). A magnetic dipole model explains the observed period and period-derivative for a highly magnetized ($\sim 10^8$G), hot subdwarf of typical mass $\sim 0.5M_\odot$ and radius $\sim 0.3R_\odot$, and an age of $\sim 3\times 10^4$yr. The subdwarf spin is close to its breakup speed and its spindown luminosity is near its Eddington limit, likely as a result of accretion from a companion.

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Abraham Loeb, Dan Maoz. 2022-02-10. A Hot Subdwarf Model for the 18.18 Minute Pulsar GLEAM-X. https://arxiv.org/abs/2202.04949

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