PSR J0453+1559 may be a neutron star–white dwarf binary, study suggests

On: October 7, 2019

PSR J0453+1559 may be a neutron star–white dwarf binary, study suggests
Astronomers have investigated a compact binary radio pulsar system known as PSR J0453+1559, with the aim of shedding more light on its mysterious nature. The new study, published September 26 on arXiv.org, challenges previous assumptions, suggesting that system contains a white dwarf companion.
phys.org
Go to Source

Previous Post: Search for gravitational waves from a long-lived remnant of the binary neutron star merger GW170817. (arXiv:1810.02581v2 [gr-qc] UPDATED)

Next Post: Scientists observe year-long plateaus in decline of Type Ia supernova light curves