Search Publications

The evidence for unusually high hydrogen abundances in the central part of Valles Marineris on Mars
DOI: 10.1016/j.icarus.2021.114805 Bibcode: 2022Icar..37414805M

Mitrofanov, I.; Zelenyi, L.; Malakhov, A. +6 more

Studies of hydrogen deposition in the shallow Martian subsurface have been conducted by two neutron and one gamma-ray detectors in the past and provided global hydrogen maps (Boynton et al., 2002; Feldman et al., 2002; Mitrofanov et al., 2002). It is known from these maps that hydrogen is most abundant in the polar permafrost areas compared to the…

2022 Icarus
ExoMars-16 17
Relationship between Ca and Hα chromospheric emission in F-G-K stars: Indication of stellar filaments?
DOI: 10.1051/0004-6361/202142120 Bibcode: 2022A&A...658A..57M

Kretzschmar, M.; Meunier, N.; Delfosse, X. +2 more

Context. Different relationships between the Hα and Ca II chromospheric emissions have been reported in solar-type stars. In particular, the time-series of emissions in these two lines are clearly anti-correlated for a few percent of the stars, contrary to what is observed on the Sun.
Aims: Our objective is to characterise these relationships…

2022 Astronomy and Astrophysics
SOHO 17
The eROSITA Final Equatorial-Depth Survey (eFEDS). Variability catalogue and multi-epoch comparison
DOI: 10.1051/0004-6361/202141155 Bibcode: 2022A&A...661A...8B

Schmitt, J. H. M. M.; Georgakakis, A.; Salvato, M. +10 more

The 140-square-degrees Final Equatorial-Depth Survey (eFEDS) field, observed with the extended ROentgen Survey with an Imaging Telescope Array (eROSITA) on board the Spectrum-Roentgen-Gamma mission, provides a first look at the variable eROSITA sky. We analysed the intrinsic X-ray variability of the eFEDS sources and provide X-ray light curves and…

2022 Astronomy and Astrophysics
Gaia XMM-Newton 17
Bulge formation inside quiescent lopsided stellar disks: Connecting accretion, star formation, and morphological transformation in a z ∼ 3 galaxy group
DOI: 10.1051/0004-6361/202243100 Bibcode: 2022A&A...666A..44K

Daddi, Emanuele; Pety, Jérôme; Tan, Qinghua +10 more

We present well-resolved near-IR and submillimeter analysis of the three highly star-forming massive (> 1011 M) galaxies within the core of the RO-1001 galaxy group at z = 2.91. Each of them displays kpc scale compact starbursting cores with properties consistent with forming galaxy bulges, embedded at the center of exten…

2022 Astronomy and Astrophysics
eHST 17
MiMO: Mixture Model for Open Clusters in Color-Magnitude Diagrams
DOI: 10.3847/1538-4357/ac5f4f Bibcode: 2022ApJ...930...44L

Li, Lu; Shao, Zhengyi

We propose a mixture model of open clusters (OCs) in color-magnitude diagrams (CMDs) to measure the OC properties, including isochrone parameters (age, distance, metallicity, and dust extinction), stellar mass function (MF), and binary parameters (binary fraction and mass-ratio distribution), with high precision and reliability. The model treats a…

2022 The Astrophysical Journal
Gaia 17
A census of OBe stars in nearby metal-poor dwarf galaxies reveals a high fraction of extreme rotators
DOI: 10.1051/0004-6361/202244730 Bibcode: 2022A&A...667A.100S

Lennon, D. J.; Schootemeijer, A.; Langer, N. +3 more

The early Universe, together with many nearby dwarf galaxies, is deficient in heavy elements. The evolution of massive stars in such environments is thought to be affected by rotation. Extreme rotators among them tend to form decretion disks and manifest themselves as OBe stars. We use a combination of UB, Gaia, Spitzer, and Hubble Space Telescope…

2022 Astronomy and Astrophysics
Gaia eHST 17
The eccentric millisecond pulsar, PSR J0955−6150. I. Pulse profile analysis, mass measurements, and constraints on binary evolution
DOI: 10.1051/0004-6361/202142670 Bibcode: 2022A&A...665A..53S

Camilo, F.; Possenti, A.; Kramer, M. +17 more

Context. PSR J0955−6150 is a member of an enigmatic class of eccentric millisecond pulsar (MSP) and helium white dwarf (He WD) systems (eMSPs), whose binary evolution is poorly understood and believed to be strikingly different to that of traditional MSP+He WD systems in circular orbits.
Aims: Measuring the masses of the stars in this system …

2022 Astronomy and Astrophysics
Gaia 17
Single-lens mass measurement in the high-magnification microlensing event Gaia19bld located in the Galactic disc
DOI: 10.1051/0004-6361/202039542 Bibcode: 2022A&A...657A..18R

Harrison, D. L.; Bryden, G.; Soszyński, I. +66 more

Context. Microlensing provides a unique opportunity to detect non-luminous objects. In the rare cases that the Einstein radius θE and microlensing parallax πE can be measured, it is possible to determine the mass of the lens. With technological advances in both ground- and space-based observatories, astrometric and interferom…

2022 Astronomy and Astrophysics
Gaia 17
Interstellar Neutrals, Pickup Ions, and Energetic Neutral Atoms Throughout the Heliosphere: Present Theory and Modeling Overview
DOI: 10.1007/s11214-022-00883-6 Bibcode: 2022SSRv..218...18S

Zank, Gary P.; Zhang, Ming; Mostafavi, Parisa +11 more

Interstellar neutrals (ISNs), pick-up ions (PUIs), and energetic neutral atoms (ENAs) are fundamental constituents of the heliosphere and its interaction with the neighboring interstellar medium. Here, we focus on selected aspects of present-day theory and modeling of these particles. In the last decades, progress in the understanding of the role …

2022 Space Science Reviews
Ulysses 17
Finding Quasars behind the Galactic Plane. II. Spectroscopic Identifications of 204 Quasars at ∣b∣ < 20°
DOI: 10.3847/1538-4365/ac7f3e Bibcode: 2022ApJS..261...32F

Zheng, Jie; Jiang, Linhua; Feng, Xiaotong +21 more

Quasars behind the Galactic plane (GPQs) are important astrometric references and valuable probes of Galactic gas, yet the search for GPQs is difficult due to severe extinction and source crowding in the Galactic plane. In this paper, we present a sample of 204 spectroscopically confirmed GPQs at ∣b∣ < 20°, 191 of which are new discoveries. Thi…

2022 The Astrophysical Journal Supplement Series
Gaia 17