The origin of the bright and hard X-ray emission flux among the
We report the discovery of ZTF J0127+5258, a compact mass-transferring binary with an orbital period of 13.7 minutes. The system contains a white dwarf accretor, which likely originated as a post–common envelope carbon–oxygen (CO) white dwarf, and a warm donor (
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- DOI PREFIX: 10.3847
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- Journal Name:
- The Astrophysical Journal Letters
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- Article No. L1
- Medium: X
- Sponsoring Org:
- National Science Foundation
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The origin of the bright and hard X-ray emission flux among the
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The detonation of an overlying helium layer on a 0.8–1.1
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