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The extremely X-ray luminous radio-loud quasar CFHQS J142952 + 544717 at z = 6.18 under Chandra high-angular resolution lens
DOI: 10.1093/mnras/stad1959 Bibcode: 2023MNRAS.524.1087M

Cheung, C. C.; Stawarz, Ł.; Siemiginowska, A. +6 more

We present the first X-ray observation at sub-arcsecond resolution of the high-redshift (z = 6.18) radio-loud quasar CFHQS J142952 + 544717 (J1429). The ~100 net-count 0.3-7 keV spectrum obtained from ~30 ks Chandra exposure is best fit by a single power-law model with a photon index Γ = 2.0 ± 0.2 and no indication of an intrinsic absorber, implyi…

2023 Monthly Notices of the Royal Astronomical Society
XMM-Newton 8
Distillation of 56Fe in Ultramassive O-Ne White Dwarfs
DOI: 10.3847/1538-4357/acbfaa Bibcode: 2023ApJ...946...78C

Blouin, Simon; Caplan, Matthew E.; Freeman, Ian F.

When white dwarfs freeze, the plasma mixtures inside them undergo separation processes that can produce radical changes in the composition profile of the star. The abundance of neutron-rich elements, such as 22Ne or 56Fe, determines whether or not the first crystals are more or less dense than the surrounding fluid and thus w…

2023 The Astrophysical Journal
Gaia 8
Physical Properties of 5000 Cool Large Magellanic Cloud Supergiants with Gaia XP Spectra: A Detailed Portrait of the Upper H-R Diagram Hints at Missing Supernova Progenitors
DOI: 10.3847/1538-4357/ad0725 Bibcode: 2023ApJ...959..102D

Dorn-Wallenstein, Trevor Z.; Levesque, Emily M.; Neugent, Kathryn F.

Characterizing the physical properties of cool supergiants allows us to probe the final stages of a massive star's evolution before it undergoes core collapse. Despite their importance, the fundamental properties of these stars- $\mathrm{log}{T}_{\mathrm{eff}}$ and $\mathrm{log}L/{L}_{\odot }$ -are only known for a limited number of objects. The t…

2023 The Astrophysical Journal
Gaia 8
The first look at narrow-line Seyfert 1 galaxies with eROSITA
DOI: 10.1051/0004-6361/202244620 Bibcode: 2023A&A...669A..37G

Salvato, M.; Buchner, J.; Boller, Th. +6 more

We present the first look at the spectral and timing analysis of narrow-line Seyfert 1 galaxies (NLS1s) with the extended ROentgen Survey with an Imaging Telescope Array (eROSITA) on board the Spectrum-Roentgen-Gamma (SRG) mission. The sample of approximately 1200 NLS1s was obtained via a cross-match between the first eROSITA All-Sky Survey (eRASS…

2023 Astronomy and Astrophysics
XMM-Newton 8
V445 Puppis: Dustier than a Thousand Novae
DOI: 10.3847/2041-8213/acdf56 Bibcode: 2023ApJ...952L..26B

Evans, A.; Banerjee, D. P. K.; Starrfield, S. +4 more

V445 Puppis, the only known Galactic helium nova, is a unique test bed to verify supernova (SN) theories in the single-degenerate channel that involve a white dwarf (WD) accreting matter from a helium-rich donor. An estimate of the mass of the helium shell on the WD is crucial to deciding whether or not it will undergo an SN detonation. In this co…

2023 The Astrophysical Journal
AKARI Herschel 8
Probing Ganymede's Atmosphere with HST Lyα Images in Transit of Jupiter
DOI: 10.3847/PSJ/acaf7f Bibcode: 2023PSJ.....4...12R

Saur, Joachim; Roth, Lorenz; Becker, Tracy M. +6 more

We report results from far-ultraviolet observations by the Hubble Space Telescope of Jupiter's largest moon, Ganymede, transiting across the planet's dayside hemisphere. Within a targeted campaign on 2021 September 9 two exposures were taken during one transit passage to probe for attenuation of Jupiter's hydrogen Lyα dayglow above the moon limb. …

2023 The Planetary Science Journal
eHST 8
The SOFIA FEEDBACK [CII] Legacy Survey: Rapid molecular cloud dispersal in RCW 79
DOI: 10.1051/0004-6361/202347721 Bibcode: 2023A&A...679L...5B

Schneider, N.; Zavagno, A.; Tielens, A. G. G. M. +12 more

It has long been discussed whether stellar feedback in the form of winds and/or radiation can shred the nascent molecular cloud, thereby controlling the star formation rate. However, directly probing and quantifying the impact of stellar feedback on the neutral gas of the nascent clouds is challenging. We present an investigation of this impact to…

2023 Astronomy and Astrophysics
Gaia 8
A mid-infrared study of synthetic glass and crystal mixtures analog to the geochemical terranes on mercury
DOI: 10.1016/j.icarus.2023.115498 Bibcode: 2023Icar..39615498M

Helbert, Joern; Hiesinger, Harald; Weber, Iris +8 more

The MERTIS (MErcury Radiometer and Thermal Infrared Spectrometer) onboard of the BepiColombo ESA/JAXA mission to Mercury will map the surface of Mercury in the wavelength range of 7-14 µm and for the interpretation of these spectra a database of analog materials is needed. We analyzed bulk grain size fractions of a series of analog materials…

2023 Icarus
BepiColombo 8
The Lyα Reference Sample. XIV. Lyα Imaging of 45 Low-redshift Star-forming Galaxies and Inferences on Global Emission
DOI: 10.3847/1538-4365/acc2b8 Bibcode: 2023ApJS..266...15M

Verhamme, Anne; Cannon, John M.; Hayes, Matthew +18 more

We present Lyα imaging of 45 low-redshift star-forming galaxies observed with the Hubble Space Telescope. The galaxies have been selected to have moderate to high star formation rates (SFRs) using far-ultraviolet (FUV) luminosity and Hα equivalent width criteria, but no constraints on Lyα luminosity. We employ a pixel stellar continuum fitting cod…

2023 The Astrophysical Journal Supplement Series
eHST 8
Recurrent solar density transients in the slow wind observed with the Metis coronagraph
DOI: 10.1051/0004-6361/202346623 Bibcode: 2023A&A...675A.170V

Heinzel, P.; Sasso, C.; Romoli, M. +22 more

Aims We aim to investigate and characterize the morphology and dynamics of small-scale coronal plasma density inhomogeneities detected as brighter, denser features propagating outward through the solar corona in the visible-light images of the Metis coronagraph on board Solar Orbiter on February 22, 2021. Our main focus is on investigating their p…

2023 Astronomy and Astrophysics
SolarOrbiter 8