Search Publications

Perturbed distribution functions with accurate action estimates for the Galactic disc
DOI: 10.1051/0004-6361/202040118 Bibcode: 2022A&A...658A..50A

Monari, G.; Ramos, P.; Siebert, A. +8 more

In the Gaia era, understanding the effects of the perturbations of the Galactic disc is of major importance in the context of dynamical modelling. In this theoretical paper we extend previous work in which, making use of the epicyclic approximation, the linearized Boltzmann equation had been used to explicitly compute, away from resonances, the pe…

2022 Astronomy and Astrophysics
Gaia 5
Catalog of Wide Binary, Trinary and Quaternary Candidates from the Gaia Data Release 2 (Region ∣b∣ > 25°)
DOI: 10.3847/1538-3881/ac34f9 Bibcode: 2022AJ....163...33Z

Zavada, Petr; Píška, Karel

The occurrence of multiple stars, dominantly binaries, is studied using the Gaia-ESA DR2 catalog. We apply the optimized statistical method that we previously developed for the analysis of 2D patterns. The field of stars is divided into a mosaic of small pieces that represent a statistical set for analysis. Specifically, data input is represented …

2022 The Astronomical Journal
Gaia 5
Observing EAGLE galaxies with JWST: predictions for Milky Way progenitors and their building blocks
DOI: 10.1093/mnras/stac2410 Bibcode: 2022MNRAS.516.3861E

Fattahi, Azadeh; Deason, Alis J.; Frenk, Carlos S. +1 more

We present predictions, derived from the EAGLE ΛCDM cosmological hydrodynamical simulations, for the abundance and properties of galaxies expected to be detected at high redshift by the James Webb Space Telescope (JWST). We consider the galaxy population as a whole and focus on the sub-population of progenitors of Milky Way (MW) analogues, defined…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 5
Modeling a Coronal Mass Ejection as a Magnetized Structure with EUHFORIA
DOI: 10.3847/1538-4357/ac3bd2 Bibcode: 2022ApJ...925...25S

Singh, Jagdev; Asvestari, E.; Sindhuja, G. +1 more

We studied an Earth-directed coronal mass ejection (CME) that erupted on 2015 March 15. Our aim was to model the CME flux rope as a magnetized structure using the European Heliospheric Forecasting Information Asset (EUHFORIA). The flux rope from eruption data (FRED) output was applied to the EUHFORIA spheromak CME model. In addition to the geometr…

2022 The Astrophysical Journal
SOHO 5
Millisecond Pulsars in Dense Star Clusters: Evolution, Scaling Relations, and the Galactic-center Gamma-Ray Excess
DOI: 10.3847/1538-4357/ac9cd0 Bibcode: 2022ApJ...940..162Y

Ye, Claire S.; Fragione, Giacomo

The number of millisecond pulsars (MSPs) observed in Milky Way globular clusters has increased explosively in recent years, but the underlying population is still uncertain due to observational biases. We use state-of-the-art N-body simulations to study the evolution of MSP populations in dense star clusters. These cluster models span a wide range…

2022 The Astrophysical Journal
Gaia 5
An Updated View of the Milky Way from Maser Astrometry
DOI: 10.3390/universe8080390 Bibcode: 2022Univ....8..390I

Immer, Katharina; Rygl, Kazi L. J.

Astrometric observations of maser sources in the Milky Way, using the Very Long Baseline Interferometry (VLBI) technique, have been exploited to determine the spiral structure of our Galaxy. Several major spiral arms have now been pinpointed in the first and second Galactic quadrants. Fundamental Galactic parameters such as the distance to the Gal…

2022 Universe
Gaia 5
Analysis of four solar occultations by Titan's atmosphere with the infrared channel of the VIMS instrument: Haze, CH4, CH3D, and CO vertical profiles
DOI: 10.1051/0004-6361/202243045 Bibcode: 2022A&A...666A.140R

Rannou, P.; Vinatier, S.; Coutelier, M. +1 more

Titan, the largest satellite of Saturn, has a dense atmosphere mainly composed of nitrogen, methane at a percent level, and minor species. It is also covered by a thick and global photochemical organic haze. In the last two decades, the observations made by the Cassini orbiter and the Huygens probe have greatly improved our knowledge of Titan's sy…

2022 Astronomy and Astrophysics
Cassini 5
Multiwavelength Mitigation of Stellar Activity in Astrometric Planet Detection
DOI: 10.3847/1538-3881/ac56e0 Bibcode: 2022AJ....163..205K

Solanki, Sami K.; Macintosh, Bruce; Krivova, Natalie +4 more

Astrometry has long been a promising technique for exoplanet detection. At the theoretical limits, astrometry would allow for the detection of smaller planets than previously seen by current exoplanet search methods, but stellar activity may make these theoretical limits unreachable. Astrometric jitter of a Sun-like star due to magnetic activity i…

2022 The Astronomical Journal
Gaia 5
Automated Detection of coronaL MAss Ejecta origiNs for Space Weather AppliCations (ALMANAC)
DOI: 10.1029/2022SW003253 Bibcode: 2022SpWea..2003253W

Morgan, Huw; Williams, Thomas

Alerts of potentially hazardous coronal mass ejection (CME) are based on the detection of rapid changes in remote observations of the solar atmosphere. This paper presents a method that detects and estimates the central coordinates of CME eruptions in Extreme Ultraviolet data, with the dual aim of providing an early alert, and giving an initial es…

2022 Space Weather
SOHO 5
An arid-semiarid climate during the Noachian-Hesperian transition in the Huygens region, Mars: Evidence from morphological studies of valley networks
DOI: 10.1016/j.icarus.2021.114789 Bibcode: 2022Icar..37314789S

Xiao, Long; Zhao, Jiannan; Yang, Yong +2 more

Fluvial activities play important roles in the geologic evolution of early Mars. As one of the most ancient fluvial features on Mars, the widely distributed valley networks (VNs) provide clues for understanding the early martian climate. Our study focuses on the morphological and hydrological features of VNs around the Huygens basin in the ancient…

2022 Icarus
MEx 5