output
19942026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

Showing 2018 · astro-ph.GAShow all

43 papers · 2 filters

astro-ph.GA2018★ 4 cited

How gravitational softening affects galaxy stability I. Linear mode analysis of disc galaxies

Sven De Rijcke, Jean-Baptiste Fouvry, Walter Dehnen

Linear perturbation is used to investigate the effect of gravitational softening on the retrieved two-armed spiral eigenmodes of razor-thin stellar discs. We explore four softening…

astro-ph.GA2018★ 48 cited

Space Telescope and Optical Reverberation Mapping Project. X. Understanding the Absorption-Line Holiday in NGC 5548

M. Dehghanian, G. J. Ferland, G. A. Kriss +27

The flux variations in the emission lines in active galactic nuclei (AGNs) are driven by variations in the ionizing continuum flux --which are usually reflected in the observable U…

astro-ph.GA2018★ 10 cited

The Environments of Luminous Radio - WISE Selected Infrared Galaxies

J. I. Penney, A. W. Blain, D. Wylezalek +17

We have observed the environments of a population of 33 heavily dust obscured, ultra-luminous, high-redshift galaxies, selected using WISE and NVSS at 1.3 with the Infra-Red Ar…

astro-ph.GA2018★ 67 cited

The Multiple Merger Assembly of a Hyper-luminous Obscured Quasar at redshift 4.6

T. Diaz-Santos, R. J. Assef, A. W. Blain +10

Galaxy mergers and gas accretion from the cosmic web drove the growth of galaxies and their central black holes at early epochs. We report spectroscopic imaging of a multiple merge…

astro-ph.GA2018★ 199 cited

The hidden giant: discovery of an enormous Galactic dwarf satellite in Gaia DR2

G. Torrealba, V. Belokurov, S. E. Koposov +8

We report the discovery of a Milky Way satellite in the constellation of Antlia. The Antlia 2 dwarf galaxy is located behind the Galactic disc at a latitude of a…

astro-ph.GA2018★ 8 cited

Reliable mass calculation in spherical gravitating systems

Foivos I. Diakogiannis, Geraint F. Lewis, Rodrigo A. Ibata +3

We present an innovative approach to the methodology of dynamical modelling, allowing practical reconstruction of the underlying dark matter mass without assuming both the density…