Search Publications

JWST Mid-infrared Spectroscopy Resolves Gas, Dust, and Ice in Young Stellar Objects in the Large Magellanic Cloud
DOI: 10.3847/1538-4357/ad18bc Bibcode: 2024ApJ...963...94N

Hirschauer, Alec S.; Lenkić, Laura; Meixner, Margaret +9 more

In this work, we present spectra of 11 young stellar objects (YSOs) taken with the Mid-Infrared Instrument / Medium Resolution Spectroscopy (MRS) instrument on board the James Webb Space Telescope (JWST). The YSOs are located in the N79 region of the Large Magellanic Cloud (LMC), an active star-forming region with hundreds of Spitzer- and Herschel…

2024 The Astrophysical Journal
JWST 6
Merging Signatures in an Offset Lyman Continuum Emitter at Redshift 3.8
DOI: 10.3847/1538-4357/ad75ff Bibcode: 2024ApJ...975...53Y

Zheng, Zhen-Ya; Cheng, Cheng; Yuan, Fang-Ting +3 more

Lyman continuum (LyC) emitters at z > 3 provide critical samples for studying the contribution of galaxies to the ionizing background in the epoch of reionization. We collect a sample of z > 3 LyC emitters, a dominant fraction (∼60%–70%) of which show spatial offsets between LyC emission and the nonionizing continuum. From this sample, espec…

2024 The Astrophysical Journal
eHST JWST 6
Comparative Analysis of Type III Radio Bursts and Solar Flares: Spatial Localization and Correlation with Solar Flare Intensity
DOI: 10.3847/1538-4357/ad12ba Bibcode: 2024ApJ...961...88K

Maksimovic, Milan; Szabo, Adam; Bale, Stuart D. +8 more

We present a comprehensive study of type III radio bursts and their association with solar flares of magnitude M1.0 and larger, as observed by four widely separated spacecraft (Parker Solar Probe, Solar Orbiter, STEREO-A, and Wind). Our main focus is the introduction and validation of two methods for localizing radio bursts using the available mul…

2024 The Astrophysical Journal
SolarOrbiter Ulysses 6
JWST/NIRCam Paβ Narrowband Imaging Reveals Ordinary Dust Extinction for Hα Emitters within the Spiderweb Protocluster at z = 2.16
DOI: 10.3847/1538-4357/ad8156 Bibcode: 2024ApJ...977...74P

Pérez-González, Pablo G.; Koyama, Yusei; Kodama, Tadayuki +7 more

We combine JWST/NIRCam and Subaru/MOIRCS dual Paβ+Hα narrowband imaging to trace the dust attenuation and the star formation activities of a sample of 43 Hα emitters at the core of one of the most massive and best-studied clusters in formation at the cosmic noon: the Spiderweb protocluster at z = 2.16. We find that most Hα emitters display Paβ/Hα …

2024 The Astrophysical Journal
JWST 6
A SPectroscopic Survey of Biased Halos In the Reionization Era (ASPIRE): JWST Supports Earlier Reionization around [O III] Emitters
DOI: 10.3847/1538-4357/ad82de Bibcode: 2024ApJ...976...93J

Hennawi, Joseph F.; Fan, Xiaohui; Cai, Zheng +22 more

Understanding when and how reionization happened is crucial for studying the early structure formation and the properties of the first galaxies in the Universe. At z > 5.5, the observed intergalactic medium (IGM) optical depth shows a significant scatter, indicating an inhomogeneous reionization process. However, the nature of the inhomogeneous…

2024 The Astrophysical Journal
JWST 6
Comparative Study of the Kinetic Properties of Proton and Alpha Beams in the Alfvénic Wind Observed by SWA-PAS On Board Solar Orbiter
DOI: 10.3847/1538-4357/ad47b3 Bibcode: 2024ApJ...969..106B

Telloni, Daniele; Sorriso-Valvo, Luca; Marino, Raffaele +12 more

The problems of heating and acceleration of solar wind particles are of significant and enduring interest in astrophysics. The interactions between waves and particles are crucial in determining the distributions of proton and alpha particles, resulting in non-Maxwellian characteristics, including temperature anisotropies and particle beams. These…

2024 The Astrophysical Journal
SolarOrbiter 6
Revisiting the Helium and Hydrogen Accretion Indicators at TWA 27B: Weak Mass Flow at Near-freefall Velocity
DOI: 10.3847/1538-4357/ad1ee9 Bibcode: 2024ApJ...964...70M

Zhou, Yifan; Hashimoto, Jun; Marleau, Gabriel-Dominique +1 more

TWA 27B (2M1207b) is the first directly imaged planetary-mass (M p ≈ 5 M J) companion and was observed at 0.9–5.3 µm with JWST/NIRSpec. To understand the accretion properties of TWA 27B, we search for continuum-subtracted near-infrared helium and hydrogen emission lines and measure their widths and luminosities. We dete…

2024 The Astrophysical Journal
eHST JWST 6
Resolving the Mechanical and Radiative Feedback in J1044+0353 with Keck Cosmic Web Imager Spectral Mapping
DOI: 10.3847/1538-4357/ad34ac Bibcode: 2024ApJ...966..190M

Martin, Crystal L.; Peng, Zixuan; Li, Yuan

We present integral field spectroscopy toward and around J1044+0353, a rapidly growing, low-metallicity galaxy that produces extreme [O III] line emission. A new map of the O32 flux ratio reveals a density-bounded ionization cone emerging from the starburst. The interaction of the hydrogen-ionizing radiation, produced by the very young starburst, …

2024 The Astrophysical Journal
eHST 6
A Multiwavelength, Multiepoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. II. Photometric Light Curves
DOI: 10.3847/1538-4357/ad543d Bibcode: 2024ApJ...971...96W

Kóspál, Ágnes; Calvet, Nuria; Espaillat, Catherine C. +8 more

Classical T Tauri stars (CTTSs) are young, low-mass stars that accrete material from their surrounding protoplanetary disk. To better understand accretion variability, we conducted a multiepoch, multiwavelength photometric monitoring campaign of four CTTSs, TW Hya, RU Lup, BP Tau, and GM Aur, in 2021 and 2022, contemporaneous with Hubble Space Tel…

2024 The Astrophysical Journal
eHST 6
Evidence for a Redshifted Excess in the Intracluster Light Fractions of Merging Clusters at z 0.8
DOI: 10.3847/2041-8213/ad181a Bibcode: 2024ApJ...960L...7J

Jiménez-Teja, Yolanda; Dupke, Renato A.; Dimauro, Paola +1 more

The intracluster light (ICL) fraction is a well-known indicator of the dynamical activity in intermediate-redshift clusters. Merging clusters in the redshift interval 0.18 < z < 0.56 have a distinctive peak in the ICL fractions measured between ~3800 and 4800 Å . In this work, we analyze two higher-redshift, clearly merging clusters, ACT-CLJ…

2024 The Astrophysical Journal
eHST 6