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The volcanology of Idunn Mons, Venus: The complex evolution of a possible active volcano
DOI: 10.1016/j.jvolgeores.2021.107428 Bibcode: 2022JVGR..42107428L

Komatsu, Goro; López, Iván; D'Incecco, Piero +1 more

Idunn Mons is a shield volcano located in the Imdr Regio large igneous rise, a Venusian equivalent to a hotspot geologic province on Earth. Recent studies using emissivity data from ESA's Venus Express Mission, together with experimental laboratory studies on the alteration of volcanic materials on Venus conditions, suggest that Idunn Mons is a po…

2022 Journal of Volcanology and Geothermal Research
VenusExpress 7
SRG/eROSITA view of X-ray reflection in the Central Molecular Zone: a snapshot in September-October 2019
DOI: 10.1093/mnras/stab3333 Bibcode: 2022MNRAS.509.6068K

Khabibullin, Ildar; Churazov, Eugene; Sunyaev, Rashid

X-ray reflection off dense molecular clouds in the Galactic Centre region has established itself as a powerful probe for the past activity record of the supermassive black hole Sgr A* on a time-scale of a few hundred years. Detailed studies of the reflection signal from individual clouds allow us to estimate parameters of the brightest flare(s) an…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 7
A Massive, Dusty, HI Absorption-Selected Galaxy at z ≈ 2.46 Identified in a CO Emission Survey
DOI: 10.3847/1538-4357/ac7b2c Bibcode: 2022ApJ...934...87K

Walter, F.; Prochaska, J. X.; Revalski, M. +4 more

We report a NOrthern Extended Millimeter Array (NOEMA) and Atacama Large Millimeter/submillimeter Array search for redshifted CO emission from the galaxies associated with seven high-metallicity ([M/H] ≥ -1.03) damped Lyα absorbers (DLAs) at z ≈ 1.64-2.51. Our observations yielded one new detection of CO(3-2) emission from a galaxy at z = 2.4604 u…

2022 The Astrophysical Journal
Gaia eHST 7
Discovery of NES, an Extended Tidal Structure in the Northeast of the Large Magellanic Cloud
DOI: 10.3847/1538-4357/ac602c Bibcode: 2022ApJ...931...19G

Cignoni, Michele; Ripepi, Vincenzo; Tosi, Monica +4 more

We report on the discovery of a new diffuse stellar substructure protruding for >5° from the northeastern rim of the LMC disk. The structure, which we dub the northeast structure (NES), was identified by applying a Gaussian mixture model to a sample of strictly selected candidate members of the Magellanic System, extracted from the Gaia EDR3 ca…

2022 The Astrophysical Journal
Gaia 7
Slowly Cooling White Dwarfs in NGC 6752
DOI: 10.3847/1538-4357/ac7a45 Bibcode: 2022ApJ...934...93C

Cadelano, Mario; Pallanca, Cristina; Dalessandro, Emanuele +6 more

Recently, a new class of white dwarfs ("slowly cooling WDs") has been identified in the globular cluster M13. The cooling time of these stars is increased by stable thermonuclear hydrogen burning in their residual envelope. These WDs are thought to be originated by horizontal branch (HB) stars populating the HB blue tail that skipped the asymptoti…

2022 The Astrophysical Journal
eHST 7
GJ 3090 b: one of the most favourable mini-Neptune for atmospheric characterisation
DOI: 10.1051/0004-6361/202243975 Bibcode: 2022A&A...665A..91A

Bouchy, F.; Helled, R.; Mao, S. +37 more

We report the detection of GJ 3090 b (TOI-177.01), a mini-Neptune on a 2.9-day orbit transiting a bright (K = 7.3 mag) M2 dwarf located at 22 pc. The planet was identified by the Transiting Exoplanet Survey Satellite and was confirmed with the High Accuracy Radial velocity Planet Searcher radial velocities. Seeing-limited photometry and speckle im…

2022 Astronomy and Astrophysics
Gaia 7
Global dynamics and architecture of the Kepler-444 system
DOI: 10.1051/0004-6361/202243971 Bibcode: 2022A&A...667A.128S

Delisle, J. -B.; Udry, S.; Bourrier, V. +3 more

Context. S-type planets, which orbit one component of multiple-star systems, place strong constraints on planet formation and evolution models. A notable case study is Kepler-444, a triple-star system whose primary is orbited by five planets smaller than Venus in a compact configuration, and for which the stellar binary companion revolves around t…

2022 Astronomy and Astrophysics
Gaia 7
Modelling multiwavelength emission of Ultra-luminous X-ray Sources accreting above the Eddington limit
DOI: 10.1093/mnras/stab3240 Bibcode: 2022MNRAS.509.4694A

Wolter, A.; Pintore, F.; Zampieri, L. +1 more

We model the multiwavelength properties of binaries accreting at super-critical rates with the aim to better understand the observational properties of Ultra-luminous X-ray Sources (ULXs). We calculate an extended grid of binary systems which evolve through Roche Lobe Overflow and undergo case A mass transfer from massive donors (up to 25 ${\rm M}…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 7
Kinetic properties of collisionless magnetic reconnection in space plasma: in situ observations
DOI: 10.1007/s41614-022-00079-z Bibcode: 2022RvMPP...6...15Z

Zhou, Meng; Deng, Xiaohua; Zhong, Zhihong

In collisionless plasmas, magnetic reconnection is widely recognized as one of the most important energy conversion and dissipation processes. Although reconnection is usually manifested as macroscopic effects, such as large-scale magnetic topology change and fast plasma flows, kinetic physics is the underlying process driving these macroscopic ph…

2022 Reviews of Modern Plasma Physics
Cluster 7
Orbits and Occultation Opportunities of 15 TNOs Observed by New Horizons
DOI: 10.3847/PSJ/ac3491 Bibcode: 2022PSJ.....3...23P

Singer, Kelsi N.; Stern, S. Alan; Fraser, Wesley C. +10 more

We present high-precision orbits for 15 trans-Neptunian objects (TNOs) that have been observed by NASA's New Horizons spacecraft at distances from 0.092 to 2.2 au. We also give predictions of 66 future opportunities to observe stellar occultations by them in late 2021-2029, eight of which are possible to observe from the United States. Observation…

2022 The Planetary Science Journal
Gaia eHST 7