Search Publications

Signatures of the resonances of a large Galactic bar in local velocity space
DOI: 10.1051/0004-6361/201834820 Bibcode: 2019A&A...626A..41M

Monari, G.; Siebert, A.; Famaey, B. +2 more

The second data release of the Gaia mission has revealed a very rich structure in local velocity space. In terms of in-plane motions, this rich structure is also seen as multiple ridges in the actions of the axisymmetric background potential of the Galaxy. These ridges are probably related to a combination of effects from ongoing phase-mixing and …

2019 Astronomy and Astrophysics
Gaia 93
ALMA Unveils Widespread Molecular Gas Clumps in the Ram Pressure Stripped Tail of the Norma Jellyfish Galaxy
DOI: 10.3847/1538-4357/ab3e6c Bibcode: 2019ApJ...883..145J

Fumagalli, Michele; Brinks, Elias; Combes, Françoise +8 more

We present the first high-resolution map of the cold molecular gas distribution as traced by CO(2-1) emission with ALMA in a long ram pressure stripped tail. The Norma cluster galaxy ESO 137-001 is undergoing a strong interaction with the surrounding intracluster medium and is one of the nearest jellyfish galaxies with a long multiphase and multic…

2019 The Astrophysical Journal
eHST 93
The Herschel Dwarf Galaxy Survey. II. Physical conditions, origin of [C II] emission, and porosity of the multiphase low-metallicity ISM
DOI: 10.1051/0004-6361/201834457 Bibcode: 2019A&A...626A..23C

Lebouteiller, V.; Madden, S. C.; Galliano, F. +7 more

The sensitive infrared telescopes, Spitzer and Herschel, have been used to target low-metallicity star-forming galaxies, allowing us to investigate the properties of their interstellar medium (ISM) in unprecedented detail. Interpretation of the observations in physical terms relies on careful modeling of those properties. We have employed a multip…

2019 Astronomy and Astrophysics
Herschel 93
Using Gaia DR2 to constrain local dark matter density and thin dark disk
DOI: 10.1088/1475-7516/2019/04/026 Bibcode: 2019JCAP...04..026B

Buch, Jatan; Leung, John Shing Chau; Fan, JiJi

We use stellar kinematics from the latest Gaia data release (DR2) to measure the local dark matter (DM) density ρDM in a heliocentric cylinder of radius R= 150 pc and half-height z= 200 pc. We also explore the prospect of using our analysis to estimate the DM density in local substructure by setting constraints on the surface density an…

2019 Journal of Cosmology and Astroparticle Physics
Gaia 93
BAT AGN Spectroscopic Survey. XI. The Covering Factor of Dust and Gas in Swift/BAT Active Galactic Nuclei
DOI: 10.3847/1538-4357/aaef8f Bibcode: 2019ApJ...870...31I

Ueda, Yoshihiro; Kawamuro, Taiki; Ricci, Claudio +10 more

We quantify the luminosity contribution of active galactic nuclei (AGNs) to the 12 µm, mid-infrared (MIR; 5-38 µm), and total IR (5-1000 µm) emission in the local AGNs detected in the all-sky 70 month Swift/Burst Alert Telescope (BAT) ultrahard X-ray survey. We decompose the IR spectral energy distributions (SEDs) of 587 objects …

2019 The Astrophysical Journal
AKARI Herschel 93
A rapidly changing jet orientation in the stellar-mass black-hole system V404 Cygni
DOI: 10.1038/s41586-019-1152-0 Bibcode: 2019Natur.569..374M

Soria, Roberto; Sarazin, Craig L.; Jonker, Peter G. +18 more

Powerful relativistic jets are one of the main ways in which accreting black holes provide kinetic feedback to their surroundings. Jets launched from or redirected by the accretion flow that powers them are expected to be affected by the dynamics of the flow, which for accreting stellar-mass black holes has shown evidence for precession1

2019 Nature
INTEGRAL 93
The ultra-diffuse galaxy NGC 1052-DF2 with MUSE. I. Kinematics of the stellar body
DOI: 10.1051/0004-6361/201834909 Bibcode: 2019A&A...625A..76E

Emsellem, Eric; Müller, Oliver; Lelli, Federico +14 more

The so-called ultra-diffuse galaxy NGC 1052-DF2 was announced to be a galaxy lacking dark matter based on a spectroscopic study of its constituent globular clusters. Here we present the first spectroscopic analysis of the stellar body of this galaxy using the MUSE integral-field spectrograph at the (ESO) Very Large Telescope. The MUSE datacube sim…

2019 Astronomy and Astrophysics
eHST 93
The gravitational force field of the Galaxy measured from the kinematics of RR Lyrae in Gaia
DOI: 10.1093/mnras/stz572 Bibcode: 2019MNRAS.485.3296W

Gerhard, Ortwin; Wegg, Christopher; Bieth, Marie

From a sample of 15651 RR Lyrae with accurate proper motions in Gaia DR2, we measure the azimuthally averaged kinematics of the inner stellar halo between 1.5 and 20 kpc from the Galactic centre. We find that their kinematics are strongly radially anisotropic, and their velocity ellipsoid nearly spherically aligned over this volume. Only in the in…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 92
The Optical Afterglow of GW170817: An Off-axis Structured Jet and Deep Constraints on a Globular Cluster Origin
DOI: 10.3847/2041-8213/ab3d9e Bibcode: 2019ApJ...883L...1F

Berger, E.; Chornock, R.; Laskar, T. +25 more

We present a revised and complete optical afterglow light curve of the binary neutron star merger GW170817, enabled by deep Hubble Space Telescope (HST) F606W observations at ≈584 days post-merger, which provide a robust optical template. The light curve spans ≈110-362 days, and is fully consistent with emission from a relativistic structured jet …

2019 The Astrophysical Journal
eHST 92
The halo's ancient metal-rich progenitor revealed with BHB stars
DOI: 10.1093/mnras/stz853 Bibcode: 2019MNRAS.486..378L

Belokurov, Vasily; Evans, N. Wyn; Koposov, Sergey E. +2 more

Using the data from the Sloan Digital Sky Survey and the Gaia satellite, we assemble a pure sample of ∼3000 blue horizontal branch (BHB) stars with 7D information, including positions, velocities, and metallicities. We demonstrate that, as traced with BHBs, the Milky Way's stellar halo is largely unmixed and cannot be well represented with a conve…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 92