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A DZ white dwarf with a 30 MG magnetic field
DOI: 10.1093/mnras/stad143 Bibcode: 2023MNRAS.520.3560H

Hermes, J. J.; Hollands, M. A.; Stopkowicz, S. +3 more

Magnetic white dwarfs with field strengths below 10 MG are easy to recognize since the Zeeman splitting of spectral lines appears proportional to the magnetic field strength. For fields ≳100 MG, however, transition wavelengths become chaotic, requiring quantum-chemical predictions of wavelengths and oscillator strengths with a non-perturbative tre…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 12
Carbon Dioxide Retrievals From NOMAD-SO on ESA's ExoMars Trace Gas Orbiter and Temperature Profiles Retrievals With the Hydrostatic Equilibrium Equation: 1. Description of the Method
DOI: 10.1029/2022JE007277 Bibcode: 2023JGRE..12807277T

Aoki, S.; Vandaele, A. C.; Daerden, F. +14 more

The Solar Occultation (SO) channel of the Nadir and Occultation for Mars Discovery (NOMAD) instrument has been scanning the Martian atmosphere for almost 2 Martian years. In this work, we present a subset of the NOMAD SO data measured at the mesosphere at the terminator. From the data set, we investigated 968 vertical profiles of carbon dioxide de…

2023 Journal of Geophysical Research (Planets)
ExoMars-16 12
Investigating the Magnetic Structure of Interplanetary Coronal Mass Ejections Using Simultaneous Multispacecraft In Situ Measurements
DOI: 10.3847/1538-4357/acef16 Bibcode: 2023ApJ...957...49R

Farrugia, C. J.; Galvin, A. B.; Davies, E. E. +5 more

In situ measurements from spacecraft typically provide a time series at a single location through coronal mass ejections (CMEs), and they have been one of the main methods to investigate CMEs. The CME properties derived from these in situ measurements are affected by temporal changes that occur as the CME passes over the spacecraft, such as radial…

2023 The Astrophysical Journal
SolarOrbiter 12
Charging of free-falling test masses in orbit due to cosmic rays: Results from LISA Pathfinder
DOI: 10.1103/PhysRevD.107.062007 Bibcode: 2023PhRvD.107f2007A

Mendes, L.; Russano, G.; Nofrarias, M. +72 more

A comprehensive summary of the measurements made to characterize test-mass charging due to the space environment during the LISA Pathfinder mission is presented. Measurements of the residual charge of the test mass after release by the grabbing and positioning mechanism show that the initial charge of the test masses was negative after all release…

2023 Physical Review D
INTEGRAL LISAPathfinder 12
Electron Heating Scales in Collisionless Shocks Measured by MMS
DOI: 10.1029/2022GL100400 Bibcode: 2023GeoRL..5000400J

Johlander, Andreas; Khotyaintsev, Yuri V.; Dimmock, Andrew P. +2 more

Electron heating at collisionless shocks in space is a combination of adiabatic heating due to large-scale electric and magnetic fields and non-adiabatic scattering by high-frequency fluctuations. The scales at which heating happens hints to what physical processes are taking place. In this letter, we study electron heating scales with data from t…

2023 Geophysical Research Letters
Cluster 12
Splitting the lentils: Clues to galaxy/black hole coevolution from the discovery of offset relations for non-dusty versus dusty (wet-merger-built) lenticular galaxies in the Mbh-M*,spheroid and Mbh-M*,galaxy diagrams
DOI: 10.1093/mnras/stad529 Bibcode: 2023MNRAS.521.1023G

Graham, Alister W.

This work advances the (galaxy morphology)-dependent (black hole mass, Mbh)-(spheroid/galaxy stellar mass, M*) scaling relations by introducing 'dust bins' for lenticular (S0) galaxies. Doing so has led to the discovery of Mbh-M*,sph and Mbh-M*,gal relations for dusty S0 galaxies - …

2023 Monthly Notices of the Royal Astronomical Society
eHST 12
The Magellanic Edges Survey - IV. Complex tidal debris in the SMC outskirts
DOI: 10.1093/mnrasl/slac129 Bibcode: 2023MNRAS.518L..25C

Da Costa, G. S.; Koposov, S. E.; Mackey, A. D. +2 more

We use data from the Magellanic Edges Survey (MagES) in combination with Gaia EDR3 to study the extreme southern outskirts of the Small Magellanic Cloud (SMC), focussing on a field at the eastern end of a long arm-like structure which wraps around the southern periphery of the Large Magellanic Cloud (LMC). Unlike the remainder of this structure, w…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 12
A radio-jet-driven outflow in the Seyfert 2 galaxy NGC 2110?
DOI: 10.1051/0004-6361/202245408 Bibcode: 2023A&A...675A..58P

Rigopoulou, D.; Hönig, S. F.; Villar-Martín, M. +16 more

We present a spatially resolved study of the ionized gas in the central 2 kpc of the Seyfert 2 galaxy NGC 2110 and investigate the role of its moderate-luminosity radio jet (kinetic radio power of Pjet = 2.3 × 1043 erg s−1). We used new optical integral-field observations taken with the MEGARA spectrograph at the G…

2023 Astronomy and Astrophysics
Gaia eHST 12
The VLT MUSE NFM view of outflows and externally photoevaporating discs near the orion bar
DOI: 10.1093/mnras/stad2581 Bibcode: 2023MNRAS.525.4129H

Bally, John; Reiter, Megan; Manara, Carlo F. +10 more

We present Very Large Telescope/Multi-Unit Spectroscopic Explorer Narrow Field Mode observations of a pair of disc-bearing young stellar objects towards the Orion Bar: 203-504 and 203-506. Both of these discs are subject to external photoevaporation, where winds are launched from their outer regions due to environmental irradiation. Intriguingly, …

2023 Monthly Notices of the Royal Astronomical Society
Gaia 12
Catalog of Planetary Nebulae Detected by GALEX and Corollary Optical Surveys
DOI: 10.3847/1538-4365/acca77 Bibcode: 2023ApJS..266...34G

Bianchi, L.; Gómez-Muñoz, M. A.; Manchado, A.

Planetary nebulae (PNs) consist of an ionized envelope surrounding a hot central star (CSPN) that emits mostly at ultraviolet (UV) wavelengths. UV observations, therefore, provide important information on both the CSPN and the nebula. We have matched the PNs in the Hong Kong/Australian Astronomical Observatory/Strasbourg Hα catalog with the Galaxy…

2023 The Astrophysical Journal Supplement Series
Gaia IUE 12