Search Publications

On the origins of backscattered solar wind energetic neutral hydrogen from the Moon and Mercury
DOI: 10.1016/j.pss.2023.105660 Bibcode: 2023P&SS..22905660L

Verkercke, S.; Leblanc, F.; Tramontina, D. +8 more

The surfaces of planetary airless bodies are directly bombarded by solar particles. The most abundant of those particles are solar wind protons. In the case of the Moon, many in situ observations have shown that a significant portion of these incident solar-wind protons are backscattered as energetic neutral hydrogen atoms (ENA). Measurements of t…

2023 Planetary and Space Science
Chandrayaan-1 8
Modern Estimates of the Mass of the Milky Way
DOI: 10.1134/S1063772923080024 Bibcode: 2023ARep...67..812B

Bobylev, V. V.; Baykova, A. T.

A review of various methods used to estimate the mass of the Galaxy is given. Results obtained from the analysis of the galactic rotation curve, from the kinematics of dwarf satellite galaxies of the Milky Way, from globular clusters, from trails of dwarf galaxies, from distant halo stars, from escape velocities, from the dynamics of the Local Gro…

2023 Astronomy Reports
Gaia 8
Astrochemical models of interstellar ices: History matters
DOI: 10.1051/0004-6361/202346188 Bibcode: 2023A&A...675A.165C

Gratier, P.; Dartois, E.; Noble, J. A. +6 more

Context. Ice is ubiquitous in the interstellar medium. As soon as it becomes slightly opaque in the visible, it can be seen for visual extinctions (AV) above ~1.5. The James Webb Space Telescope (JWST) will observe the ice composition toward hundreds of lines of sight, covering a broad range of physical conditions in these extinct regio…

2023 Astronomy and Astrophysics
Herschel 8
Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Diverse outcomes of binary-disk interactions
DOI: 10.1051/0004-6361/202245577 Bibcode: 2023A&A...672A.145Z

Zhang, Yapeng; Bae, Jaehan; Huang, Jane +15 more

Context. Circumstellar disks play an essential role in the outcomes of planet formation. Disks do not evolve in isolation, as about half of solar-type stars were born in binary or multiple systems. The presence of stellar companions modifies the morphology and evolution of disks, potentially resulting in a different planet population. Resolving di…

2023 Astronomy and Astrophysics
Gaia eHST 8
Planets Across Space and Time (PAST). IV. The Occurrence and Architecture of Kepler Planetary Systems as a Function of Kinematic Age Revealed by the LAMOST-Gaia-Kepler Sample
DOI: 10.3847/1538-3881/ad0368 Bibcode: 2023AJ....166..243Y

Dong, Subo; Zong, Weikai; Zhu, Zi +7 more

One of the fundamental questions in astronomy is how planetary systems form and evolve. Measuring the planetary occurrence and architecture as a function of time directly addresses this question. In the fourth paper of the Planets Across Space and Time series, we investigate the occurrence and architecture of Kepler planetary systems as a function…

2023 The Astronomical Journal
Gaia 8
Exploring the brown dwarf desert with precision radial velocities and Gaia DR3 astrometric orbits
DOI: 10.1051/0004-6361/202347578 Bibcode: 2023A&A...680A..16U

Holl, B.; Sahlmann, J.; Ségransan, D. +4 more

Context. The observed scarcity of brown dwarfs in close orbits (within 10 au) around solar-type stars has posed significant questions about the origins of these substellar companions. These questions not only pertain to brown dwarfs but also impact our broader understanding of planetary formation processes. However, to resolve these formation mech…

2023 Astronomy and Astrophysics
Gaia 8
Unravelling the mass spectrum of destroyed dwarf galaxies with the metallicity distribution function
DOI: 10.1093/mnras/stad535 Bibcode: 2023MNRAS.520.6091D

Grand, Robert J. J.; Fattahi, Azadeh; Koposov, Sergey E. +1 more

Accreted stellar populations are comprised of the remnants of destroyed galaxies, and often dominate the 'stellar haloes' of galaxies such as the Milky Way (MW). This ensemble of external contributors is a key indicator of the past assembly history of a galaxy. We introduce a novel statistical method that uses the unbinned metallicity distribution…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 8
Constraints on monopole-dipole potential from tests of gravity
DOI: 10.1103/PhysRevD.108.103024 Bibcode: 2023PhRvD.108j3024P

Poddar, Tanmay Kumar; Pachhar, Debashis

An ultralight axion like particle (ALP) can mediate a macroscopic force with long-range monopole-dipole interactions between the Earth and the Sun, if the Earth is treated as a polarized source. Because of the geomagnetic field, there exists an estimated 1042 polarized electrons within the Earth. These electrons, in a polarized state, c…

2023 Physical Review D
Gaia 8
First VLTI/GRAVITY Observations of HIP 65426 b: Evidence for a Low or Moderate Orbital Eccentricity
DOI: 10.3847/1538-3881/ad06b7 Bibcode: 2023AJ....166..257B

Lutz, D.; Genzel, R.; Sturm, E. +96 more

Giant exoplanets have been directly imaged over orders of magnitude of orbital separations, prompting theoretical and observational investigations of their formation pathways. In this paper, we present new VLTI/GRAVITY astrometric data of HIP 65426 b, a cold, giant exoplanet which is a particular challenge for most formation theories at a projecte…

2023 The Astronomical Journal
Gaia Hipparcos JWST 8
Ca triplet metallicities and velocities for 12 globular clusters toward the galactic bulge
DOI: 10.1051/0004-6361/202244959 Bibcode: 2023A&A...669A.115G

Minniti, D.; Saviane, I.; Geisler, D. +6 more

Context. Globular clusters (GCs) are excellent tracers of the formation and early evolution of the Milky Way. The bulge GCs (BGCs) are particularly important because they can reveal vital information about the oldest in situ component of the Milky Way.
Aims: Our aim is to derive the mean metallicities and radial velocities for 13 GCs that lie…

2023 Astronomy and Astrophysics
Gaia 8