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Antaeus: A Retrograde Group of Tidal Debris in the Milky Way's Disk Plane
DOI: 10.3847/2041-8213/ac86d3 Bibcode: 2022ApJ...936L...3O

Martin, Nicolas; Famaey, Benoit; Viswanathan, Akshara +5 more

We present the discovery of a wide retrograde moving group in the disk plane of the Milky Way using action-angle coordinates derived from the Gaia DR3 catalog. The structure is identified from a sample of its members that are currently almost at the pericenter of their orbit and are passing through the solar neighborhood. The motions of the stars …

2022 The Astrophysical Journal
Gaia 16
MICROSCOPE satellite and its drag-free and attitude control system
DOI: 10.1088/1361-6382/ac09cd Bibcode: 2022CQGra..39t4003R

Bergé, Joel; Chhun, Ratana; Métris, Gilles +14 more

This paper focuses on the description of the design and performance of the MICROSCOPE satellite and its drag-free and attitude control system. The satellite is derived from CNES' Myriade platform family, albeit with significant upgrades dictated by the unprecedented MICROSCOPE's mission requirements. The 300 kg drag-free microsatellite has complet…

2022 Classical and Quantum Gravity
MICROSCOPE 16
To E or Not to E : Numerical Nuances of Global Coronal Models
DOI: 10.3847/1538-4365/ac8eb1 Bibcode: 2022ApJS..263...18B

Poedts, Stefaan; Perri, Barbara; Lani, Andrea +2 more

In recent years, global coronal models have experienced an ongoing increase in popularity as tools for forecasting solar weather. Within the domain of up to 21.5 R , magnetohydrodynamics (MHD) is used to resolve the coronal structure using magnetograms as inputs at the solar surface. Ideally, these computations would be repeated with e…

2022 The Astrophysical Journal Supplement Series
SOHO 16
Hot Jupiters, cold kinematics. High phase space densities of host stars reflect an age bias
DOI: 10.1051/0004-6361/202140921 Bibcode: 2022A&A...658A.199M

Mustill, Alexander J.; Davies, Melvyn B.; Lambrechts, Michiel

Context. The birth environments of planetary systems are thought to influence planet formation and orbital evolution through external photoevaporation and stellar flybys. Recent work has claimed observational support for this, in the form of a correlation between the properties of planetary systems and the local Galactic phase space density of the…

2022 Astronomy and Astrophysics
Gaia 16
Quantitative spectroscopy of B-type supergiants
DOI: 10.1051/0004-6361/202243973 Bibcode: 2022A&A...668A..92W

Butler, K.; Weßmayer, D.; Przybilla, N.

Context. B-type supergiants are versatile tools to address a number of highly-relevant astrophysical topics, ranging from stellar atmospheres over stellar and galactic evolution to the characterisation of interstellar sightlines and to the cosmic distance scale.
Aims: A hybrid non-local thermodynamic equilibrium (LTE) approach, involving line…

2022 Astronomy and Astrophysics
Gaia IUE 16
A double-peaked Lyman-α emitter with a stronger blue peak multiply imaged by the galaxy cluster RXC J0018.5+1626
DOI: 10.1093/mnras/stac2169 Bibcode: 2022MNRAS.516.1373F

Charlot, Stéphane; Bradač, Maruša; Strait, Victoria +10 more

We report the discovery of a double-peaked Lyman-α (Ly α) emitter (LAE) at z = 3.2177 ± 0.0001 in VLT/MUSE data. The galaxy is strongly lensed by the galaxy cluster RXC J0018.5+1626 recently observed in the RELICS survey, and the double-peaked Ly α emission is clearly detected in the two counter images in the MUSE field of view. We measure a relat…

2022 Monthly Notices of the Royal Astronomical Society
eHST 16
Modeling Balmer line signatures of stellar CMEs
DOI: 10.1093/mnras/stac1284 Bibcode: 2022MNRAS.513.6058L

Heinzel, P.; Odert, P.; Leitzinger, M.

From the Sun, we know that coronal mass ejections (CMEs) are a transient phenomenon, often correlated with flares. They have an impact on solar mass- and angular momentum loss, and therefore solar evolution, and make a significant part of space weather. The same is true for stars, but stellar CMEs are still not well constrained, although new metho…

2022 Monthly Notices of the Royal Astronomical Society
eHST 16
Dissecting Nearby Galaxies with piXedfit. II. Spatially Resolved Scaling Relations among Stars, Dust, and Gas
DOI: 10.3847/1538-4357/ac7da4 Bibcode: 2022ApJ...935...98A

Tacchella, Sandro; Wu, Po-Feng; Morishita, Takahiro +5 more

We study spatially resolved scaling relations among stars, dust, and gas in ten nearby spiral galaxies. In a preceding paper, we have derived spatially resolved properties of the stellar population and dust by a panchromatic spectral energy distribution fitting using piXedfit. Now, we investigate resolved star formation ( ${{\rm{\Sigma }}}_{{{\rm{…

2022 The Astrophysical Journal
Herschel 16
The whisper of a whimper of a bang: 2400 d of the Type Ia SN 2011fe reveals the decay of 55Fe
DOI: 10.1093/mnras/stac2873 Bibcode: 2022MNRAS.517.4119T

Kochanek, C. S.; Stanek, K. Z.; Ashall, C. +4 more

We analyse new multifilter Hubble Space Telescope (HST) photometry of the normal Type Ia supernova (SN Ia) 2011fe out to ≈2400 d after maximum light, the latest observations to date of a SN Ia. We model the pseudo-bolometric light curve with a simple radioactive decay model and find energy input from both 57Co and 55Fe are ne…

2022 Monthly Notices of the Royal Astronomical Society
eHST 16
Coronal mass ejection followed by a prominence eruption and a plasma blob as observed by Solar Orbiter
DOI: 10.1051/0004-6361/202243162 Bibcode: 2022A&A...665A...7B

Heinzel, P.; Mierla, M.; Zhukov, A. N. +26 more

Context. On 2021 February 12, two subsequent eruptions occurred above the western limb of the Sun, as seen along the Sun-Earth line. The first event was a typical slow coronal mass ejection (CME), followed ∼7 h later by a smaller and collimated prominence eruption, originating south of the CME, followed by a plasma blob. These events were observed…

2022 Astronomy and Astrophysics
SOHO SolarOrbiter 16