output
20052024
most citedGravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

3.6k citations

Showing 2016Show all

17 papers · 1 filter

astro-ph.EP2016★ 24 cited

Stellar and planetary Cassini states

Alexandre C. M. Correia

Cassini states correspond to equilibria of the spin axis of a body when its orbit is perturbed. They were initially described for satellites, but the spin axis of stars and planets…

astro-ph.HE2016★ 134 cited

The distribution of radioactive Ti in Cassiopeia A

Brian W. Grefenstette, Chris L. Fryer, Fiona A. Harrison +28

The distribution of elements produced in the inner-most layers of a supernova explosion is a key diagnostic for studying the collapse of massive stars. Here we present the results…

astro-ph.GA2016★ 37 cited

Herschel / HIFI spectral line survey of the Orion Bar - Temperature and density differentiation near the PDR surface

Z. Nagy, Y. Choi, V. Ossenkopf-Okada +7

Photon Dominated Regions (PDRs) are interfaces between the mainly ionized and mainly molecular material around young massive stars. Analysis of the physical and chemical structure…

astro-ph.GA2016★ 91 cited

Millimeter-Wave Line Ratios and Sub-beam Volume Density Distributions

Adam K. Leroy, Antonio Usero, Andreas Schruba +11

We explore the use of mm-wave emission line ratios to trace molecular gas density when observations integrate over a wide range of volume densities within a single telescope beam.…

astro-ph.GA2016★ 140 cited

The VIMOS Public Extragalactic Redshift Survey (VIPERS): Galaxy segregation inside filaments at

N. Malavasi, S. Arnouts, D. Vibert +42

We present the first quantitative detection of large-scale filamentary structure at in the large cosmological volume probed by the VIMOS Public Extragalactic Redshif…

astro-ph.EP2016★ 24 cited

Study and application of the resonant secular dynamics beyond Neptune

Melaine Saillenfest, Marc Fouchard, Giacomo Tommei +1

We use a secular representation to describe the long-term dynamics of transneptunian objects in mean-motion resonance with Neptune. The model applied is thoroughly described in Sai…