Radio Continuum Studies of Ultracompact and Short Orbital Period X-Ray Binaries
We present the radio continuum counterparts to the enigmatic ultracompact X-ray binaries (UCXBs): a black hole or neutron star accreting from a hydrogen-deficient white dwarf donor star with short orbital periods (<80 minutes). For the sample of UCXBs hosted by globular clusters (GCs), we search for whether certain GC properties are more likely to
Dage, Kristen C. et al.
Fecha de publicación:
7
2025