PSR J1930-1852: a pulsar in the widest known orbit around another neutron star
arXiv:1503.06276 · doi:10.1088/0004-637X/805/2/156
Abstract
In the summer of 2012, during a Pulsar Search Collaboratory workshop, two high-school students discovered J19301852, a pulsar in a double neutron star (DNS) system. Most DNS systems are characterized by short orbital periods, rapid spin periods and eccentric orbits. However, J19301852 has the longest spin period (185 ms) and orbital period (45 days) yet measured among known, recycled pulsars in DNS systems, implying a shorter than average and/or inefficient recycling period before its companion went supernova. We measure the relativistic advance of periastron for J19301852, (4) deg/yr, which implies a total mass (M(4) M) consistent with other DNS systems. The constraints on M place limits on the pulsar and companion masses ( M and M respectively). J19301852's spin and orbital parameters challenge current DNS population models and make J19301852 an important system for further investigation.
8 pages, 6 figures
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