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First Joint MUSE, Hubble Space Telescope, and JWST Spectrophotometric Analysis of the Intracluster Light: The Case of the Relaxed Cluster RX J2129.7+0005
DOI: 10.3847/1538-4357/ad701b Bibcode: 2024ApJ...974..309J

Koekemoer, Anton M.; Hjorth, Jens; Jiménez-Teja, Yolanda +8 more

We present the most detailed spectrum of intracluster light (ICL) in an individual cluster to date, the relaxed system RX J2129.7+0005, at z ∼ 0.234. Using 15 broadband, deep images observed with the Hubble Space Telescope and JWST in the optical and the infrared, plus deep integral field spectroscopy from MUSE, we computed a total of 3696 ICL map…

2024 The Astrophysical Journal
eHST JWST 1
Unraveling the Origins of an Extreme Solar Eruptive Event with Hard X-Ray Imaging Spectroscopy
DOI: 10.3847/1538-4357/ad57b7 Bibcode: 2024ApJ...972...48V

Krucker, Säm; Vourlidas, Angelos; Vievering, Juliana T.

Hard X-ray (HXR) observations are crucial for understanding the initiation and evolution of solar eruptive events, as they provide a key signature of flare-accelerated electrons and heated plasma. The potential of high-cadence HXR imaging for deciphering the erupting structure, however, has not received adequate attention in an era of extreme ultr…

2024 The Astrophysical Journal
SolarOrbiter 1
Revisiting the Chemical Composition of WD 1145+017: Impact of Circumstellar Disk Contamination on Photospheric Abundances
DOI: 10.3847/1538-4357/ad90b7 Bibcode: 2024ApJ...977...93L

Dufour, Patrick; Xu, Siyi; Le Bourdais, Érika

We performed a chemical analysis of the asteroid-bearing white dwarf WD 1145+017 using optical and ultraviolet spectroscopic data from 25 epochs between 2015 and 2023. We present an updated gas disk model with improved opacity calculations and temperature profiles to properly account for all circumstellar absorption features. Incorporating these c…

2024 The Astrophysical Journal
eHST 1
Detailed Abundances of the Planet-hosting TOI-1173 A/B System: Possible Evidence of Planet Engulfment in a Very Wide Binary
DOI: 10.3847/1538-4357/ad697f Bibcode: 2024ApJ...974..122Y

McWilliam, Andrew; Simon, Joshua D.; Reggiani, Henrique +7 more

Over the last decade, studies of large samples of binary systems have identified chemical anomalies and shown that they might be attributed to planet formation or planet engulfment. However, both scenarios have primarily been tested in pairs without known exoplanets. In this work, we explore these scenarios in the newly detected planet-hosting wid…

2024 The Astrophysical Journal
Gaia 1
Sensitivity of the Helioglow to Variation of the Total Ionization Rate and Solar Lyα Emission
DOI: 10.3847/1538-4357/ad2a55 Bibcode: 2024ApJ...965...30K

Bzowski, M.; Kubiak, M. A.; Kowalska-Leszczynska, I. +1 more

Direct observations of solar wind are mostly limited to the vicinity of the ecliptic plane. Retrieving the latitudinal structure of solar wind indirectly based on observations of the backscatter glow of interstellar neutral hydrogen is complex and requires support from theoretical models. The GLOWS instrument, to operate on the planned IMAP missio…

2024 The Astrophysical Journal
SOHO 1
Tracking an Eruptive Prominence Using Multiwavelength and Multiview Observations on 2023 March 7
DOI: 10.3847/1538-4357/ad8bad Bibcode: 2024ApJ...977....4Z

Song, Yongliang; Huang, Zhenghua; Zhang, Qingmin +2 more

In this paper, we carry out multiwavelength and multiview observations of the prominence eruption, which generated a C2.3 class flare and a coronal mass ejection (CME) on 2023 March 7. For the first time, we apply the revised cone model to three-dimensional reconstruction and tracking of the eruptive prominence for ∼4 hr. The prominence propagates…

2024 The Astrophysical Journal
SOHO SolarOrbiter 1
Chandra X-Ray Observations of PSR J1849-0001, Its Pulsar Wind Nebula, and the TeV Source HESS J1849-000
DOI: 10.3847/1538-4357/ad3e6d Bibcode: 2024ApJ...968...67G

Kargaltsev, Oleg; Klingler, Noel; Yang, Hui +4 more

We obtained a 108 ks Chandra X-ray Observatory (CXO) observation of PSR J1849-0001 and its pulsar wind nebula (PWN) coincident with the TeV source HESS J1849-000. By analyzing the new and old (archival) CXO data, we resolved the pulsar from the PWN, explored the PWN morphology on arcsecond and arcminute scales, and measured the spectra of differen…

2024 The Astrophysical Journal
Gaia 1
Atmospheric Abundances and Bulk Properties of the Binary Brown Dwarf Gliese 229Bab from JWST/MIRI Spectroscopy
DOI: 10.3847/2041-8213/ad92f9 Bibcode: 2024ApJ...977L..32X

Zhang, Yapeng; Perrin, Marshall D.; Knutson, Heather A. +8 more

We present JWST/Mid Infrared Instrument (MIRI) low-resolution spectroscopy (4.75–14 µm) of the first known substellar companion, Gliese 229Bab, which was recently resolved into a tight binary brown dwarf. Previous atmospheric retrieval studies modeling Gliese 229B as a single brown dwarf have reported anomalously high carbon-to-oxygen ratios…

2024 The Astrophysical Journal
JWST 1
Determining the Nanoflare Heating Frequency of an X-Ray Bright Point Observed by MaGIXS
DOI: 10.3847/1538-4357/ad2766 Bibcode: 2024ApJ...967...23M

Reeves, Katharine K.; Del Zanna, Giulio; Golub, Leon +18 more

Nanoflares are thought to be one of the prime candidates that can heat the solar corona to its multimillion kelvin temperature. Individual nanoflares are difficult to detect with the present generation of instruments, but their presence can be inferred by comparing simulated nanoflare-heated plasma emissions with the observed emission. Using HYDRA…

2024 The Astrophysical Journal
Hinode 1
Stellar Characterization and a Chromospheric Activity Analysis of a K2 Sample of Planet-hosting Stars
DOI: 10.3847/1538-4357/ad4b15 Bibcode: 2024ApJ...970...53L

Cunha, Katia; Smith, Verne V.; Quispe-Huaynasi, F. +4 more

Effective temperatures, surface gravities, and iron abundances were derived for 109 stars observed by the K2 mission using equivalent width measurements of Fe I and Fe II lines. Calculations were carried out in local thermodynamic equilibrium using Kurucz model atmospheres. Stellar masses and radii were derived by combining the stellar parameters …

2024 The Astrophysical Journal
Gaia 1