Pulsar preprints for 11-09-2018

Submitted by Astro-ph Robot on Tue, 09/11/2018 - 20:47

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"Numerical simulations of mass loading in the tails of Bow Shock Pulsar Wind Nebulae."

Barbara Olmi, Niccolò Bucciantini, Giovanni Morlino.

"Disentangling Coalescing Neutron Star-White Dwarf Binaries for LISA."

Thomas M. Tauris.

"GW$\times$LSS: Chasing the Progenitors of Merging Binary Black Holes."

Giulio Scelfo, Nicola Bellomo, Alvise Raccanelli, Sabino Matarrese, Licia Verde.

"Digging the population of compact binary mergers out of the noise."

Sebastian M. Gaebel, John Veitch, Thomas Dent, Will M. Farr.

"How frequent are close supermassive binary black holes in powerful jet sources?."

Martin G. H. Krause, Stanislav S. Shabala, Martin J. Hardcastle, Geoffrey V. Bicknell, Hans Böhringer, Gayoung Chon, Mohammad A. Nawaz, Marc Sarzi, Alexander Y. Wagner.

"An Analytical Portrait of Binary Mergers in Hierarchical Triple Systems."

Lisa Randall, Zhong-Zhi Xianyu.

"Probing non-Gaussian Stochastic Gravitational Wave Backgrounds with LISA."

Nicola Bartolo, Valerie Domcke, Daniel G. Figueroa, Juan Garcia-Bellido, Marco Peloso, Mauro Pieroni, Angelo Ricciardone, Mairi Sakellariadou, Lorenzo Sorbo, Gianmassimo Tasinato.

"The host galaxies of double compact objects merging in the local Universe."

Michela Mapelli, Nicola Giacobbo, Mattia Toffano, Emanuele Ripamonti, Alessandro Bressan, Mario Spera, Marica Branchesi.

"Neutron Star Mergers Might not be the Only Source of r-Process Elements in the Milky Way."

Benoit Côté, Marius Eichler, Almudena Arcones, Camilla J. Hansen, Paolo Simonetti, Anna Frebel, Chris L. Fryer, Marco Pignatari, Moritz Reichert, Francesca Matteucci.

"A NuSTAR observation of the low mass X-ray binary GX 349+2 throughout the Z-track."

Benjamin M. Coughenour, Edward M. Cackett, Jon M. Miller, Renee M. Ludlam.

"Stochastic Chemical Evolution of Galactic Subhalos and the Origin of r-Process Elements."

Takuya Ojima, Yuhri Ishimaru, Shinya Wanajo, Nikos Prantzos, Patrick Francois.

"Physical conditions for the r-process I. radioactive energy sources of kilonovae."

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