Search Publications

The host galaxy of GRB 980425/SN1998bw: a collisional ring galaxy
DOI: 10.1093/mnras/stz735 Bibcode: 2019MNRAS.485.5411A

Le Floc'h, E.; Pian, E.; Bournaud, F. +8 more

We report Giant Metrewave Radio Telescope (GMRT), Very Large Telescope (VLT), and Spitzer Space Telescope observations of ESO 184-G82, the host galaxy of GRB 980425/SN 1998bw, that yield evidence of a companion dwarf galaxy at a projected distance of 13 kpc. The companion, hereafter GALJ193510-524947, is a gas-rich, star-forming galaxy with a star…

2019 Monthly Notices of the Royal Astronomical Society
eHST 22
A study of cool white dwarfs in the Sloan Digital Sky Survey Data Release 12
DOI: 10.1093/mnras/sty2751 Bibcode: 2019MNRAS.482..649O

Kepler, S. O.; Koester, D.; Ourique, G. +2 more

In this work, we study white dwarfs where 30 000 K > T_{eff} > 5000 K to compare the differences in the cooling of DAs and non-DAs and their formation channels. Our final sample is composed by nearly 13 000 DAs and more than 3 000 non-DAs that are simultaneously in the SDSS DR12 spectroscopic database and in the Gaia survey DR2. We present t…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 22
GIADA microbalance measurements on board Rosetta: submicrometer- to micrometer-sized dust particle flux in the coma of comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201834912 Bibcode: 2019A&A...630A..25D

Fulle, M.; Della Corte, V.; Rotundi, A. +7 more

Context. From August 2014 to September 2016, Rosetta escorted comet 67P/Churyumov-Gerasimenko (67P) during its journey around the Sun. One of the aims of Rosetta was to characterize cometary activity and the consequent formation of dust flux structures in cometary comae.
Aims: We characterize and quantify the submicrometer- to micrometer-size…

2019 Astronomy and Astrophysics
Rosetta 22
The dust in M31
DOI: 10.1093/mnras/stz2166 Bibcode: 2019MNRAS.489.5436W

Dalcanton, J. J.; Griffin, M. J.; Smith, M. W. L. +6 more

We have analysed Herschel observations of M31, using the PPMAP procedure. The resolution of PPMAP images is sufficient (∼ 31 pc on M31) that we can analyse far-IR dust emission on the scale of giant molecular clouds. By comparing PPMAP estimates of the far-IR emission optical depth at 300 µ m (τ_{{300}}), and the near-IR extinction optical d…

2019 Monthly Notices of the Royal Astronomical Society
Herschel eHST 22
A spatio-kinematic model for jets in post-AGB stars
DOI: 10.1051/0004-6361/201936073 Bibcode: 2019A&A...631A..53B

De Marco, O.; Van Winckel, H.; Kamath, D. +1 more


Aims: We aim to determine the geometry, density gradient, and velocity structure of jets in post-asymptotic giant branch (post-AGB) binaries.
Methods: Our high cadence time series of high-resolution optical spectra of jet-creating post-AGB binary systems provide us with a unique tomography of the jet. We determine the spatio-kinematic st…

2019 Astronomy and Astrophysics
Gaia 22
ACCESS: Ground-based Optical Transmission Spectroscopy of the Hot Jupiter WASP-4b
DOI: 10.3847/1538-3881/aaf9a3 Bibcode: 2019AJ....157...68B

López-Morales, Mercedes; Jordán, Andrés; Espinoza, Néstor +6 more

We present an optical transmission spectrum of the atmosphere of WASP-4b obtained through observations of four transits with Magellan/IMACS, as part of the Arizona-CfA-Católica-Carnegie Exoplanet Spectroscopy Survey (ACCESS). Using a Bayesian approach to atmospheric retrieval, we find no evidence for scattering or absorption features in our transi…

2019 The Astronomical Journal
Gaia 22
Peculiar Velocities of Galaxies Just Beyond the Local Group
DOI: 10.3847/1538-4357/ab24e5 Bibcode: 2019ApJ...880...52A

Anand, Gagandeep S.; Shaya, Edward J.; Tully, R. Brent +2 more

The Milky Way lies in a thin plane, the Local Sheet, a part of a wall bounding the Local Void lying toward the north supergalactic pole. Galaxies with accurate distances both above and below this supergalactic equatorial plane have systematically negative peculiar velocities. The interpretation of this situation is that the Local Void is expanding…

2019 The Astrophysical Journal
eHST 22
Close Cassini flybys of Saturn's ring moons Pan, Daphnis, Atlas, Pandora, and Epimetheus
DOI: 10.1126/science.aat2349 Bibcode: 2019Sci...364.2349B

Brown, R. H.; Baines, K. H.; Buratti, B. J. +35 more

Saturn's main ring system is associated with a set of small moons that either are embedded within it or interact with the rings to alter their shape and composition. Five close flybys of the moons Pan, Daphnis, Atlas, Pandora, and Epimetheus were performed between December 2016 and April 2017 during the ring-grazing orbits of the Cassini mission. …

2019 Science
Cassini 22
A-type stars in the Canada-France Imaging Survey - II. Tracing the height of the disc at large distances with Blue Stragglers
DOI: 10.1093/mnras/sty3334 Bibcode: 2019MNRAS.483.3119T

Laporte, Chervin F. P.; McConnachie, Alan W.; Malhan, Khyati +7 more

We present the kinematics of Blue Straggler (BS) stars identified in the Canada-France Imaging Survey (CFIS), covering 4000 deg2 on the sky in the u band. The BSs sample, characterized through CFIS and Pan-STARRS photometry, has been kinematically decomposed into putative halo and disc populations after cross-matching with Gaia astromet…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 22
Metallicity dependence of the Hercules stream in Gaia/RAVE data - explanation by non-closed orbits
DOI: 10.1093/mnras/stz266 Bibcode: 2019MNRAS.484.4540H

Hattori, Kohei; Kumamoto, Jun; Tagawa, Hiromichi +4 more

The origin of the Hercules stream, the most prominent velocity substructure in the Solar neighbour disc stars, is still under debate. Recent accurate measurements of position, velocity, and metallicity provided by Tycho Gaia Astrometric Solution (TGAS) and RAdial Velocity Experiments (RAVE) have revealed that the Hercules stream is most clearly se…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 22