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MHD study of the planetary magnetospheric response during extreme solar wind conditions: Earth and exoplanet magnetospheres applications
DOI: 10.1051/0004-6361/202141181 Bibcode: 2022A&A...659A..10V

Pantellini, F.; Zarka, P.; Varela, J. +3 more

Context. The stellar wind and the interplanetary magnetic field modify the topology of planetary magnetospheres. Consequently, the hazardous effect of the direct exposition to the stellar wind, for example, regarding the integrity of satellites orbiting the Earth or the habitability of exoplanets, depends upon the space weather conditions.
Ai…

2022 Astronomy and Astrophysics
Cluster 13
The stellar 'Snake' - I. Whole structure and properties
DOI: 10.1093/mnras/stac843 Bibcode: 2022MNRAS.513..503W

Fang, Min; Wang, Fan; Tian, Haijun +10 more

To complement our previous discovery of the young snake-like structure in the solar neighbourhood and reveal the structure's full extent, we build two samples of stars within the Snake and its surrounding territory from Gaia Early Data Release 3 (EDR3). With the friends-of-friends algorithm, we identify 2694 and 9052 Snake member candidates from t…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13
Molecular gas properties of Planck-selected protocluster candidates at z ≃ 1.3-3
DOI: 10.1051/0004-6361/202142255 Bibcode: 2022A&A...662A..85P

Kneissl, R.; Dole, H.; Frye, B. L. +3 more

We report on IRAM 30-m/EMIR observations of 38 Herschel sources chosen as the brightest red submillimeter (submm) sources in 18 Planck-selected fields drawn from the Planck high-z (PHz) sample of protocluster candidates. These fields host overdensities of red Herschel sources, with high star formation rates (∼10 000 M yr−1),…

2022 Astronomy and Astrophysics
Herschel 13
MICROSCOPE instrument description and validation
DOI: 10.1088/1361-6382/ac1619 Bibcode: 2022CQGra..39t4002L

Bergé, Joel; Chhun, Ratana; Métris, Gilles +19 more

This paper focuses on the dedicated accelerometers developed for the MICROSCOPE mission taking into account the specific range of acceleration to be measured on board the satellite. Considering one micro-g and even less as the full range of the instrument with an objective of one femto-g resolution, that leads to a customized concept and a high-pe…

2022 Classical and Quantum Gravity
MICROSCOPE 13
Galactic Mass Estimates Using Dwarf Galaxies as Kinematic Tracers
DOI: 10.3847/1538-4357/ac390b Bibcode: 2022ApJ...924..131S

Eadie, Gwendolyn; Slizewski, Anika; Dufresne, Xander +4 more

New mass estimates and cumulative mass profiles with Bayesian credible regions for the Milky Way (MW) are found using the Galactic Mass Estimator (GME) code and dwarf galaxy (DG) kinematic data from multiple sources. GME takes a hierarchical Bayesian approach to simultaneously estimate the true positions and velocities of the DGs, their velocity a…

2022 The Astrophysical Journal
Gaia 13
Kinematic Structure of the Large Magellanic Cloud Globular Cluster System from Gaia eDR3 and Hubble Space Telescope Proper Motions
DOI: 10.3847/1538-4357/ac81c9 Bibcode: 2022ApJ...935..149B

van der Marel, Roeland P.; Alfaro-Cuello, Mayte; Watkins, Laura L. +3 more

We have determined bulk proper motions (PMs) for 31 LMC GCs from Gaia eDR3 and Hubble Space Telescope data using multiple independent analysis techniques. Combined with literature values for distances, line-of-sight velocities, and existing bulk PMs, we extract full 6D phase-space information for 32 clusters, allowing us to examine the kinematics …

2022 The Astrophysical Journal
Gaia eHST 13
The Wave Telescope Technique
DOI: 10.1029/2021JA030165 Bibcode: 2022JGRA..12730165N

Glassmeier, K. -H.; Narita, Y.; Motschmann, U.

Unambiguous determination of wavevectors (wavelengths and propagation directions) is one of the major challenges of space plasma observations, since conventional wave analysis methods for the single spacecraft data are limited to the time series data analysis and the wave properties are determined as a function of the frequencies in the spacecraft…

2022 Journal of Geophysical Research (Space Physics)
Cluster 13
Improved Orbital Constraints and Hα Photometric Monitoring of the Directly Imaged Protoplanet Analog HD 142527 B
DOI: 10.3847/1538-3881/ac73f4 Bibcode: 2022AJ....164...29B

Weinberger, Alycia J.; De Rosa, Robert J.; Pueyo, Laurent +9 more

Companions embedded in the cavities of transitional circumstellar disks have been observed to exhibit excess luminosity at Hα, an indication that they are actively accreting. We report 5 yr (2013-2018) of monitoring of the position and Hα excess luminosity of the embedded, accreting low-mass stellar companion HD 142527 B from the MagAO/VisAO instr…

2022 The Astronomical Journal
Gaia 13
Dynamical masses for two M1 + mid-M dwarf binaries monitored during the SPHERE-SHINE survey
DOI: 10.1051/0004-6361/202142438 Bibcode: 2022A&A...658A.145B

Henning, T.; Messina, S.; D'Orazi, V. +25 more

We present orbital fits and dynamical masses for HIP 113201AB and HIP 36985AB, two M1 + mid-M dwarf binary systems monitored as part of the SPHERE-SHINE survey. To robustly determine the age of both systems via gyrochronology, we undertook a photometric monitoring campaign for HIP 113201 and GJ 282AB, the two wide K star companions to HIP 36985, u…

2022 Astronomy and Astrophysics
Gaia Hipparcos 13
The structure and 3D kinematics of vela OB2
DOI: 10.1093/mnras/stac3101 Bibcode: 2022MNRAS.517.5704A

Wright, Nicholas J.; Cantat-Gaudin, Tristan; Jeffries, R. D. +2 more

The kinematics of stars in OB associations can provide insights into their formation, dynamical evolution, and eventual fate. The low-mass stellar content of OB associations are sufficiently numerous as to provide a detailed sampling of their kinematic properties, however spectroscopy is required to confirm the youth of individual stars and to get…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13