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Breaking the Radio - Gamma-Ray Connection in Arp 220
Tova M. Yoast-Hull, Norman Murray
Recent analyses of the gamma-ray spectrum from the ultra-luminous infrared galaxy Arp 220 have revealed a discrepancy in the cosmic ray energy injection rates derived from the gamm…
GW170817: A Neutron Star Merger in a Mass-Transferring Triple System
Philip Chang, Norman Murray
The light curve of GW170817 is surprisingly blue and bright. Assuming that the event is a binary neutron star merger, we argue that blueness and brightness of the light curve is th…
Bright transients from strongly-magnetized neutron star-black hole mergers
Daniel J. D'Orazio, Janna Levin, Norman W. Murray +1
Direct detection of black hole-neutron star pairs is anticipated with the advent of aLIGO. Electromagnetic counterparts may be crucial for a confident gravitational-wave detection…
Insights into Tidal Disruption of Stars from PS1-10jh
Linda E. Strubbe, Norman Murray
Was PS1-10jh (Gezari et al. 2012), an optical/UV transient discovered by the Pan-STARRS Medium Deep Survey, the tidal disruption of a star by a massive black hole? We address two a…
On the Dynamics of Ultra Compact X-ray Binaries: 4U 1850-087, 4U 0513-40 and M15 X-2
Snezana Prodan, Norman Murray
In this work we extend our dynamical study of Ultra Compact X-ray Binaries (UCXB) 4U 1820-30 from Prodan and Murray 2012 to three more UCXBs in globular clusters: 4U 1850-087, 4U 0…
Black hole triple dynamics: breakdown of the orbit average approximation and implications for gravitational wave detections
Fabio Antonini, Norman Murray, Seppo Mikkola
Coalescing black hole (BH) binaries forming in the dense core of globular clusters (GCs) are expected to be one the brightest sources of gravitational wave (GW) radiation for the n…