Search Publications

Multistage Reconnection Powering a Solar Coronal Jet
DOI: 10.3847/1538-4357/acb0c9 Bibcode: 2023ApJ...944...19L

Teriaca, Luca; Long, David M.; Berghmans, David +5 more

Coronal jets are short-lived eruptive features commonly observed in polar coronal holes and are thought to play a key role in the transfer of mass and energy into the solar corona. We describe unique contemporaneous observations of a coronal blowout jet seen by the Extreme Ultraviolet Imager (EUI) on board the Solar Orbiter (SO) spacecraft and the…

2023 The Astrophysical Journal
SolarOrbiter 8
Untangling the Sources of Abundance Dispersion in Low-metallicity Stars
DOI: 10.3847/1538-4357/aca659 Bibcode: 2023ApJ...944...47G

Weinberg, David H.; Johnson, Jennifer A.; Ilyin, Ilya +4 more

We measure abundances of 12 elements (Na, Mg, Si, Ca, Sc, Ti, V, Cr, Mn, Fe, Co, Ni) in a sample of 86 metal-poor (-2 ≲ [Fe/H] ≲ -1) subgiant stars in the solar neighborhood. Abundances are derived from high-resolution spectra taken with the Potsdam Echelle Polarimetric and Spectroscopic Instrument on the Large Binocular Telescope, modeled using i…

2023 The Astrophysical Journal
Gaia 8
CLEAR: Spatially Resolved Emission Lines and Active Galactic Nuclei at 0.6 < z < 1.3
DOI: 10.3847/1538-4357/aca668 Bibcode: 2023ApJ...943...37B

Papovich, Casey; Cleri, Nikko J.; Holwerda, Benne W. +8 more

We investigate spatially resolved emission-line ratios in a sample of 219 galaxies (0.6 < z < 1.3) detected using the G102 grism on the Hubble Space Telescope Wide Field Camera 3 taken as part of the CANDELS Lyα Emission at Reionization survey to measure ionization profiles and search for low-luminosity active galactic nuclei (AGN). We analy…

2023 The Astrophysical Journal
eHST 8
Discovery of A Large-scale Bent Radio Jet in the Merging Cluster A514
DOI: 10.3847/2041-8213/acffc8 Bibcode: 2023ApJ...957L...4L

Kale, Ruta; Lee, Wonki; ZuHone, John +3 more

We report a discovery of a large-scale bent radio jet in the merging galaxy cluster A514 (z = 0.071). The radio emission originates from the two radio lobes of the active galactic nucleus (AGN) located near the center of the southern subcluster and extends toward the southern outskirts with multiple bends. Its peculiar morphology is characterized …

2023 The Astrophysical Journal
XMM-Newton 8
Macrospicules and Their Connection to Magnetic Reconnection in the Lower Solar Atmosphere
DOI: 10.3847/2041-8213/acac2b Bibcode: 2023ApJ...942L..22D

Shen, Yuandeng; Zhou, Xinping; Duan, Yadan +4 more

Solar macrospicules are beam-like cool plasma ejections of size in between spicules and coronal jets, which can elucidate potential connections between plasma jetting activity at different scales. With high-resolution observations from the New Vacuum Solar Telescope and Solar Dynamics Observatory, we investigate the origin of five groups of recurr…

2023 The Astrophysical Journal
IRIS 8
Constraining the White-dwarf Mass and Magnetic Field Strength of a New Intermediate Polar through X-Ray Observations
DOI: 10.3847/1538-4357/ace90c Bibcode: 2023ApJ...954..138V

Hailey, Charles J.; Mori, Kaya; Ramsay, Gavin +9 more

We report timing and broadband spectral analysis of a Galactic X-ray source, CXOGBS J174517.0-321356 (J1745), with a 614 s periodicity. Chandra discovered the source in the direction of the Galactic Bulge. Gong proposed that J1745 was either an intermediate polar (IP) with a mass of ~1 M , or an ultracompact X-ray binary (UCXB). To con…

2023 The Astrophysical Journal
XMM-Newton 8
Comparing Globular Cluster System Properties with Host Galaxy Environment
DOI: 10.3847/1538-4357/ace340 Bibcode: 2023ApJ...953..154H

Ma, Chung-Pei; Greene, Jenny E.; Blakeslee, John P. +2 more

We present Hubble Space Telescope photometry in the optical (F475X) and near-infrared (F110W) bands of the globular cluster (GC) systems of the inner halos of a sample of 15 massive elliptical galaxies. The targets are selected from the volume-limited MASSIVE survey, and chosen to sample a range of environments from sparsely populated groups to th…

2023 The Astrophysical Journal
eHST 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
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