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Homologous Accelerated Electron Beams, a Quasiperiodic Fast-propagating Wave, and a Coronal Mass Ejection Observed in One Fan-spine Jet
DOI: 10.3847/2041-8213/ac4df2 Bibcode: 2022ApJ...926L..39D

Shen, Yuandeng; Zhou, Chengrui; Zhou, Xinping +3 more

Using imaging and radio multi-wavelength observations, we studied the origin of two homologous accelerated electron beams and a quasiperiodic fast-propagating (QFP) wave train associated with a solar jet on 2012 July 14. The jet occurred in a small-scale fan-spine magnetic system embedded in a large-scale pseudostreamer associated with a GOES C1.4…

2022 The Astrophysical Journal
SOHO 26
Two-spacecraft detection of short-period decayless kink oscillations of solar coronal loops
DOI: 10.1093/mnras/stac2545 Bibcode: 2022MNRAS.516.5989Z

Berghmans, David; Nakariakov, Valery M.; Verbeeck, Cis +2 more

Decayless kink oscillations of an ensemble of loops are captured simultaneously by the High Resolution Imager (HRI) of the Extreme Ultraviolet Imager (EUI) and the Atmospheric Imaging Assembly (AIA) from 22:58 UT on 2021 November 5 to 00:27 UT on 2021 November 6. Oscillations are analysed by processing image sequences taken by the two instruments …

2022 Monthly Notices of the Royal Astronomical Society
SolarOrbiter 26
Single-spacecraft techniques for shock parameters estimation: A systematic approach
DOI: 10.3389/fspas.2022.1005672 Bibcode: 2022FrASS...905672T

Vainio, R.; Horbury, T.; Dresing, N. +8 more

Spacecraft missions provide the unique opportunity to study the properties of collisionless shocks utilising in situ measurements. In the past years, several diagnostics have been developed to address key shock parameters using time series of magnetic field (and plasma) data collected by a single spacecraft crossing a shock front. A critical aspec…

2022 Frontiers in Astronomy and Space Sciences
SolarOrbiter 26
Lenses In VoicE (LIVE): searching for strong gravitational lenses in the VOICE@VST survey using convolutional neural networks
DOI: 10.1093/mnras/stab3386 Bibcode: 2022MNRAS.510..500G

Vaccari, Mattia; Koopmans, Léon V. E.; Fan, Zuhui +8 more

We present a sample of 16 likely strong gravitational lenses identified in the VST Optical Imaging of the CDFS and ES1 fields (VOICE survey) using convolutional neural networks (CNNs). We train two different CNNs on composite images produced by superimposing simulated gravitational arcs on real Luminous Red Galaxies observed in VOICE. Specifically…

2022 Monthly Notices of the Royal Astronomical Society
eHST 26
Constraining SIDM with halo shapes: Revisited predictions from realistic simulations of early-type galaxies
DOI: 10.1093/mnras/stac2521 Bibcode: 2022MNRAS.516.4543D

Vogelsberger, Mark; Sparre, Martin; Zavala, Jesús +3 more

We study the effect of self-interacting dark matter (SIDM) and baryons on the shape of early-type galaxies (ETGs) and their dark matter haloes, comparing them to the predictions of the cold dark matter (CDM) scenario. We use five hydrodynamical zoom-in simulations of haloes hosting ETGs ($M_{\rm vir}\sim 10^{13}\, \mathrm{M}_{\odot }$ and $M_{*}\s…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 26
MAGAZ3NE: High Stellar Velocity Dispersions for Ultramassive Quiescent Galaxies at z ≳ 3
DOI: 10.3847/1538-4357/ac8747 Bibcode: 2022ApJ...938..109F

Cooper, M. C.; Urbano Stawinski, Stephanie M.; Muzzin, Adam +17 more

In this work, we publish stellar velocity dispersions, sizes, and dynamical masses for eight ultramassive galaxies (UMGs; $\mathrm{log}({M}_{* }/{M}_{\odot })$ > 11), z ≳ 3) from the Massive Ancient Galaxies At z > 3 NEar-infrared (MAGAZ3NE) Survey, more than doubling the number of such galaxies with velocity dispersion measurements at this …

2022 The Astrophysical Journal
eHST 26
Anomalous Cosmic Rays and Heliospheric Energetic Particles
DOI: 10.1007/s11214-022-00890-7 Bibcode: 2022SSRv..218...22G

Fichtner, H.; Leske, R. A.; Hill, M. E. +7 more

We present a review of Anomalous Cosmic Rays (ACRs), including the history of their discovery and recent insights into their acceleration and transport in the heliosphere. We focus on a few selected topics including a discussion of mechanisms of their acceleration, escape from the heliosphere, their effects on the dynamics of the heliosheath, tran…

2022 Space Science Reviews
SOHO Ulysses 26
The Drivers of the Martian Bow Shock Location: A Statistical Analysis of Mars Atmosphere and Volatile EvolutioN and Mars Express Observations
DOI: 10.1029/2021JA030147 Bibcode: 2022JGRA..12730147G

Garnier, P.; Génot, V.; Halekas, J. S. +6 more

The Martian interaction with the solar wind leads to the formation of a bow shock upstream of the planet. The shock dynamics appear complex, due to the combined influence of external and internal drivers. The extreme ultraviolet fluxes and magnetosonic Mach number are known major drivers of the shock location, while the influence of other possible…

2022 Journal of Geophysical Research (Space Physics)
MEx 26
The chemical abundance pattern of the extremely metal-poor thin disc star 2MASS J1808-5104 and its origins
DOI: 10.1093/mnras/stac2783 Bibcode: 2022MNRAS.517.3993M

Placco, Vinicius M.; Meléndez, Jorge; Roederer, Ian U. +6 more

We present a high-resolution (R ~ 35 000), high signal-to-noise (S/N = 350) Magellan/MIKE spectrum of the bright extremely metal-poor star 2MASS J1808-5104. We find [Fe/H] = -4.01 (spectroscopic LTE stellar parameters), [Fe/H] = -3.8 (photometric stellar parameters), and [Fe/H] = -3.7 (spectroscopic NLTE stellar parameters). We measured a carbon-t…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 26
The typical width of Herschel filaments
DOI: 10.1051/0004-6361/202244541 Bibcode: 2022A&A...667L...1A

Arzoumanian, D.; Palmeirim, P.; André, P. J.

Context. Dense molecular filaments are widely believed to be representative of the initial conditions of star formation in interstellar clouds. Characterizing their physical properties, such as their transverse size, is therefore of paramount importance. Herschel studies suggest that nearby (d < 500 pc) molecular filaments have a typical half-p…

2022 Astronomy and Astrophysics
Herschel 26