New public mock catalogs of Milky Way white dwarf mergers show how rates of outcomes (AM CVn, R CrB stars, SNe Ia, neutron stars) vary with binary evolution assumptions.
J., de Kool, M., & van den Heuvel, E
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Direct O-C timing analysis yields an orbital decay rate of (-1.97 ± 0.05) × 10^{-12} s s^{-1} in ZTFJ2130, from which a chirp mass of 0.408 ± 0.006 solar masses is derived assuming pure GW emission.
citing papers explorer
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The diverse outcomes of binary white dwarf mergers and connections to Galactic LISA sources
New public mock catalogs of Milky Way white dwarf mergers show how rates of outcomes (AM CVn, R CrB stars, SNe Ia, neutron stars) vary with binary evolution assumptions.
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Observing Orbital Decay in the Ultracompact Hot Subdwarf Binary System ZTFJ213056.71+442046.5
Direct O-C timing analysis yields an orbital decay rate of (-1.97 ± 0.05) × 10^{-12} s s^{-1} in ZTFJ2130, from which a chirp mass of 0.408 ± 0.006 solar masses is derived assuming pure GW emission.