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Extreme Solar Flare-driven Short-wave Fadeout Observed by SuperDARN ZHO Radar
DOI: 10.3847/1538-4357/ac6f56 Bibcode: 2022ApJ...933...45L

Wang, M.; Liu, J.; Lu, J. Y. +6 more

Based on the observations from the Super Dual Auroral Radar Network at the Zhongshan Station (-74.9 MLAT, 97.2 MLON) and GOES satellites X-ray sensor, we present the first statistical study of the dayside ionospheric short-wave fadeout (SWF) events on the Southern Hemispheric high latitude from the years 2010-2019 and provide a normal characterist…

2022 The Astrophysical Journal
SOHO 1
Erratum: Primordial black hole origin for thermal gamma-ray bursts
DOI: 10.1093/mnras/stac681 Bibcode: 2022MNRAS.512.2925D

del Barco, Oscar

2022 Monthly Notices of the Royal Astronomical Society
INTEGRAL 1
A 2+1 + 1 quadruple star system containing the most eccentric, low-mass, short-period, eclipsing binary known
DOI: 10.1093/mnras/stab3507 Bibcode: 2022MNRAS.510.2448H

Vanderburg, A.; Zasche, P.; Borkovits, T. +12 more

We present an analysis of a newly discovered 2+1 + 1 quadruple system with TESS containing an unresolved eclipsing binary (EB) as part of TIC 121088960 and a close neighbour TIC 121088959. The EB consists of two very low-mass M dwarfs in a highly eccentric (e = 0.709) short-period (P = 3.043 58 d) orbit. Given the large pixel size of TESS and the …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 1
Spectroscopic Diagnostics of the Mid-infrared Features of the Dark Globule DC 314.8-5.1 with the Spitzer Space Telescope
DOI: 10.3847/1538-4357/ac7a42 Bibcode: 2022ApJ...934...94K

Stawarz, Ł.; Rocha, W. R. M.; Kosmaczewski, E. +2 more

We present an analysis of the mid-infrared spectra, obtained from the Spitzer Space Telescope, of the dark globule DC 314.8-5.1, which is at the onset of low-mass star formation. The target has a serendipitous association with a B-type field star that illuminates a reflection nebula in the cloud. We focus on the polycyclic aromatic hydrocarbon (PA…

2022 The Astrophysical Journal
Gaia 1
The spiral density-wave structure of the Milky Way in the 3-kpc-scale solar neighbourhood: line-of-sight velocities of 252 young open clusters
DOI: 10.1093/mnras/stac426 Bibcode: 2022MNRAS.512.1169G

Gedalin, Michael; Jiang, Ing-Guey; Griv, Evgeny

Following Lin and Shu, the spiral structure in the Milky Way disc is considered as an oscillating density-wave pattern. As such, regular enhancements in density are relatedly linked to systematic variations in velocity of young stars and stellar clusters, and interstellar gas. We explain measured line-of-sight velocities of 252 open clusters with …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 1
TIC 5724661: A Long-period Binary with a Pulsating sdB Star and δ Scuti Variable
DOI: 10.3847/1538-4357/ac84d0 Bibcode: 2022ApJ...936..123J

Rappaport, Saul A.; Jayaraman, Rahul; Bieryla, Allyson +8 more

Using TESS 20 s cadence data, we have discovered an unusual combination of pulsating stars in what we infer to be a binary system. The binary consists of a standard δ Scuti star with pulsations over the range 32-41 day-1; this is in a likely wide orbit with a hot subdwarf-B (sdB) star, which itself has a large-amplitude p-mode pulsation…

2022 The Astrophysical Journal
Gaia 1
Plasma vortices driven by magnetic torsion generated by electric currents in non-magnetic planetary wakes
DOI: 10.1016/j.asr.2022.03.002 Bibcode: 2022AdSpR..69.3902D

Flandes, Alberto; Durand-Manterola, Héctor Javier

In non-collisional magnetised astrophysical plasmas, vortices can form as it is the case of the Venus plasma wake where Lundin et al. (2013) identified a large vortex through the integration of data of many orbits from the Venus Express (VEX) spacecraft. On the one hand, our purpose is to develop a theoretical foundation in order to explain the oc…

2022 Advances in Space Research
VenusExpress 1
The NuSTAR, XMM-Newton, and Suzaku View of A3395 at the Intercluster Filament Interface
DOI: 10.3847/1538-4357/ac61de Bibcode: 2022ApJ...930...83T

Wik, Daniel R.; Tombesi, Francesco; Akamatsu, Hiroki +4 more

Galaxy clusters are the largest virialized objects in the universe. Their merger dynamics and their interactions with the cosmic filaments that connect them are important for our understanding of the formation of large-scale structure. In addition, cosmic filaments are thought to possess the missing baryons in the universe. Studying the interactio…

2022 The Astrophysical Journal
XMM-Newton 1
The Radiative Gas Dynamics of Spacecraft in the Martian Atmosphere
DOI: 10.1134/S0015462822100731 Bibcode: 2022FlDy...57S.572S

Surzhikov, S. T.

The problems of the radiative gas dynamics of the Martian space vehicles MSRO, Pathfinder, and Exomars-2016 are solved using the author's custom NERAT-2D radiative-gasdynamic code. The cause of considerable heating of the rear surface of the spacecraft by heat radiation in the Martian atmosphere is studied. Calculation studies of the spectral comp…

2022 Fluid Dynamics
ExoMars-16 1
Polarimetric Behaviour of Various Lunar Impact Craters Derived from Chandrayaan-2 Dual-Frequency SAR Full-Pol L-Band Acquisitions
Bibcode: 2022LPICo2678.1916P

Das, A.; Putrevu, D.; Chakraborty, T. +4 more

Ch2 DFSAR provides the first opportunity to study Moon in L-band full-polarimetry. The paper presents results from polarimetric analysis of the impact craters.

2022 53rd Lunar and Planetary Science Conference
Chandrayaan-1 1