Search Publications

Mono-enriched stars and Galactic chemical evolution. Possible biases in observations and theory
DOI: 10.1051/0004-6361/202038805 Bibcode: 2020A&A...643A..49H

Strassmeier, K. G.; Ilyin, I.; Hansen, C. J. +9 more

A long sought after goal using chemical abundance patterns derived from metal-poor stars is to understand the chemical evolution of the Galaxy and to pin down the nature of the first stars (Pop III). Metal-poor, old, unevolved stars are excellent tracers as they preserve the abundance pattern of the gas from which they were born, and hence they ar…

2020 Astronomy and Astrophysics
Gaia 23
Kalkayotl: A cluster distance inference code
DOI: 10.1051/0004-6361/202037846 Bibcode: 2020A&A...644A...7O

Miret-Roig, N.; Bouy, H.; Casamiquela, L. +5 more

Context. The high-precision parallax data of the Gaia mission allows for significant improvements in the distance determination to stellar clusters and their stars. In order to obtain accurate and precise distance determinations, systematics such as parallax spatial correlations need to be accounted for, especially with regard to stars in small sk…

2020 Astronomy and Astrophysics
Gaia 23
A census of the nearby Pisces-Eridanus stellar stream. Commonalities with and disparities from the Pleiades
DOI: 10.1051/0004-6361/202037691 Bibcode: 2020A&A...638A...9R

Röser, Siegfried; Schilbach, Elena


Aims: Within a sphere of 400 pc radius around the Sun, we aim to search for members of the Pisces-Eridanus (Psc-Eri) stellar stream in the Gaia Data Release 2 data set. We compare basic astrophysical characteristics of the stream with those of the Pleiades.
Methods: We used a modified convergent-point method to identify stars with 2D vel…

2020 Astronomy and Astrophysics
Gaia 23
Temperature and chemical species distributions in the middle atmosphere observed during Titan's late northern spring to early summer
DOI: 10.1051/0004-6361/202038411 Bibcode: 2020A&A...641A.116V

Seignovert, B.; Teanby, N. A.; Flasar, F. M. +12 more

We present a study of the seasonal evolution of Titan's thermal field and distributions of haze, C2H2, C2H4, C2H6, CH3C2H, C3H8, C4H2, C6H6, HCN, and HC3N from March 2015 (Ls

2020 Astronomy and Astrophysics
Cassini 22
The spin-orbit alignment of visual binaries
DOI: 10.1051/0004-6361/202039138 Bibcode: 2020A&A...642A.212J

Albrecht, S.; Justesen, A. B.

Context. The angle between the stellar spin-axis and the orbital plane of a stellar or planetary companion has important implications for the formation and evolution of such systems. A study by Hale (1994, AJ, 107, 306) found that binaries with separations a ≲ 30 au are preferentially aligned while binaries on wider orbits are frequently misaligne…

2020 Astronomy and Astrophysics
Gaia 22
FEDReD. II. 3D extinction map with 2MASS and Gaia DR2 data
DOI: 10.1051/0004-6361/202037573 Bibcode: 2020A&A...641A..79H

Arenou, F.; Babusiaux, C.; Hottier, C.


Aims: We aim to map the 3D distribution of the interstellar extinction of the Milky Way disc up to distances larger than those probed with the Gaia parallax alone.
Methods: We applied the FEDReD (Field Extinction-Distance Relation Deconvolver) algorithm to the 2MASS near-infrared photometry together with the Gaia DR2 astrometry and photo…

2020 Astronomy and Astrophysics
Gaia 22
The AMBRE Project: Spectrum normalisation influence on Mg abundances in the metal-rich Galactic disc
DOI: 10.1051/0004-6361/202037522 Bibcode: 2020A&A...639A.140S

Recio-Blanco, A.; de Laverny, P.; Ordenovic, C. +2 more

Context. The abundance of α-elements provides an important fossil signature in Galactic archaeology to trace the chemical evolution of the different disc populations. High-precision chemical abundances are crucial to improving our understanding of the chemodynamical properties present in the Galaxy. However, deriving precise abundance estimations …

2020 Astronomy and Astrophysics
Gaia 22
Optical and X-ray discovery of the changing-look AGN IRAS 23226-3843 showing extremely broad and double-peaked Balmer profiles
DOI: 10.1051/0004-6361/202037897 Bibcode: 2020A&A...638A..91K

Schartel, N.; Komossa, S.; Kollatschny, W. +6 more


Aims: We detected a very strong X-ray decline in the galaxy IRAS 23226-3843 within the XMM-Newton slew survey in 2017. Subsequently, we carried out multi-band follow-up studies to investigate this fading galaxy in more detail.
Methods: We took deep follow-up Swift, XMM-Newton, and NuSTAR observations in combination with optical SALT spec…

2020 Astronomy and Astrophysics
XMM-Newton 22
Hypervelocity stars in the Gaia era. Revisiting the most extreme stars from the MMT HVS survey
DOI: 10.1051/0004-6361/202037747 Bibcode: 2020A&A...637A..53K

Heber, U.; Irrgang, A.; Kreuzer, S.

The hypervelocity star (HVS) survey conducted at the Multiple Mirror Telescope (MMT) identified 42 B-type stars in the Galactic halo whose radial velocity in the Galactic rest-frame exceeds +275 km s-1. In order to unravel the nature and origin of those high-velocity outliers, their complete six-dimensional phase space information is ne…

2020 Astronomy and Astrophysics
Gaia eHST 22
LBT transmission spectroscopy of HAT-P-12b. Confirmation of a cloudy atmosphere with no significant alkali features
DOI: 10.1051/0004-6361/201937265 Bibcode: 2020A&A...642A..98Y

Mallonn, M.; Reiners, A.; Apai, D. +10 more

The hot sub-Saturn-mass exoplanet HAT-P-12b is an ideal target for transmission spectroscopy because of its inflated radius. We observed one transit of the planet with the multi-object double spectrograph (MODS) on the Large Binocular Telescope (LBT) with the binocular mode and obtained an atmosphere transmission spectrum with a wavelength coverag…

2020 Astronomy and Astrophysics
eHST 22