Search Publications

SOPHIE velocimetry of Kepler transit candidates. XIX. The transiting temperate giant planet KOI-3680b
DOI: 10.1051/0004-6361/201834333 Bibcode: 2019A&A...623A.104H

Bouchy, F.; Deleuil, M.; Moutou, C. +15 more

Whereas thousands of transiting giant exoplanets are known today, only a few are well characterized with long orbital periods. Here we present KOI-3680b, a new planet in this category. First identified by the Kepler team as a promising candidate from the photometry of the Kepler spacecraft, we establish here its planetary nature from the radial ve…

2019 Astronomy and Astrophysics
Gaia 5
Quincuncial adaptive closed Kohonen (QuACK) map for the irregularly shaped comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201834841 Bibcode: 2019A&A...630A...1G

Grieger, B.

Context. Standard global map projections cannot display the complete surface of a highly irregular body such as the Rosetta target comet 67P/Churyumov-Gerasimenko because different points on the surface can have the same longitude and latitude.
Aims: We present a concept of generalized longitudes and latitudes that allows us to display the co…

2019 Astronomy and Astrophysics
Rosetta 5
Electron acceleration at comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201834701 Bibcode: 2019A&A...630A..40G

Nilsson, H.; Eriksson, A.; Goldstein, R. +6 more

We report the observation by the Ion and Electron Sensor (IES) of energetic (>1 keV) electrons in the plasma environment of comet 67P Churyumov-Gerasimenko (67P). Most of the electrons in the cometary coma are expected to be of solar wind, photoionization, or electron impact origin and are therefore not expected to exceed some hundreds of eV in…

2019 Astronomy and Astrophysics
Rosetta 5
CIELO-RGS: a catalog of soft X-ray ionized emission lines
DOI: 10.1051/0004-6361/201935368 Bibcode: 2019A&A...625A.122M

Grinberg, Victoria; Kretschmar, Peter; Guainazzi, Matteo +9 more

Context. High-resolution X-ray spectroscopy has advanced our understanding of the hot Universe by revealing physical properties like kinematics, temperature, and abundances of the astrophysical plasmas. Despite technical and scientific achievements, the lack of scientific products at a level higher than count spectra is hampering complete scientif…

2019 Astronomy and Astrophysics
XMM-Newton 5
Thermal X-ray emission identified from the millisecond pulsar PSR J1909-3744
DOI: 10.1051/0004-6361/201732040 Bibcode: 2019A&A...627A.141W

Guillemot, L.; Webb, N. A.; Barret, D. +5 more

Context. Pulsating thermal X-ray emission from millisecond pulsars can be used to obtain constraints on the neutron star equation of state, but to date only five such sources have been identified. Of these five millisecond pulsars, only two have well-constrained neutron star masses, which improve the determination of the radius via modelling of th…

2019 Astronomy and Astrophysics
XMM-Newton 5
J-PLUS: Discovery and characterisation of ultracool dwarfs using Virtual Observatory tools
DOI: 10.1051/0004-6361/201935256 Bibcode: 2019A&A...627A..29S

Hernández-Monteagudo, C.; Caballero, J. A.; Martín, E. L. +23 more

Context. Ultracool dwarfs are objects with spectral types equal to or later than M7. Most of them have been discovered using wide-field imaging surveys. The Virtual Observatory has proven to be very useful for efficiently exploiting these astronomical resources.
Aims: We aim to validate a Virtual Observatory methodology designed to discover a…

2019 Astronomy and Astrophysics
Gaia 5
Analysis of the origin of water, carbon monoxide, and carbon dioxide in the Uranus atmosphere
DOI: 10.1051/0004-6361/201732123 Bibcode: 2019A&A...621A.129L

Lampón, M.; Lara, L. M.; Rodrigo, R. +1 more

Context. We present here an analysis of the potential sources of oxygen species in the Uranus atmosphere.
Aims: Our aim is to explain the current measurements of H2O, CO, and CO2 in the Uranus atmosphere, which would allow us to constrain the influx of oxygen-bearing species and its origin in this planet.
Methods: W…

2019 Astronomy and Astrophysics
ISO 5
Generation of photoclinometric DTMs for application to transient changes on the surface of comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201834127 Bibcode: 2019A&A...630A..10T

Vincent, J. -B.; Hayes, A. G.; Tang, Y. +4 more

Context. The wide spatial and temporal coverage of 67P/Churyumov-Gerasimenko (67P) by the Rosetta mission has revealed a surface created by scattered large-scale changes and numerous small-scale changes. The many small-scale changes are of particular interest because they are unexpected and ubiquitous. As their topographic relief is often smaller …

2019 Astronomy and Astrophysics
Rosetta 5
Chemical composition of the outer halo globular cluster Palomar 15
DOI: 10.1051/0004-6361/201935467 Bibcode: 2019A&A...627A..70K

Rich, R. Michael; Xu, Siyi; Koch, Andreas

Globular clusters (GCs) in the outer Milky Way halo are important tracers of the assembly history of our Galaxy. Only a few of these objects show spreads in heavier elements beyond the canonical light-element variations that have essentially been found throughout the entire Galactic GC system, suggesting a more complex origin and evolution of thes…

2019 Astronomy and Astrophysics
Gaia 5
The HST Key Project galaxies NGC 1326A, NGC 1425, and NGC 4548: New variable stars and massive star population
DOI: 10.1051/0004-6361/201936074 Bibcode: 2019A&A...629A...3S

Hatzidimitriou, D.; Bonanos, A. Z.; Yang, M. +2 more

Studies of the massive star population in galaxies beyond the Local Group are the key to understanding the link between their numbers and modes of star formation in different environments. We present the analysis of the massive star population of the galaxies NGC 1326A, NGC 1425, and NGC 4548 using archival images obtained with the Hubble Space Te…

2019 Astronomy and Astrophysics
eHST 5