Search Publications

An Anisotropic Density Turbulence Model from the Sun to 1 au Derived from Radio Observations
DOI: 10.3847/1538-4357/acf6c1 Bibcode: 2023ApJ...956..112K

Kontar, Eduard P.; Chen, Xingyao; Chrysaphi, Nicolina +5 more

Solar radio bursts are strongly affected by radio-wave scattering on density inhomogeneities, changing their observed time characteristics, sizes, and positions. The same turbulence causes angular broadening and scintillation of galactic and extragalactic compact radio sources observed through the solar atmosphere. Using large-scale simulations of…

2023 The Astrophysical Journal
Cluster 18
A Candidate Runaway Supermassive Black Hole Identified by Shocks and Star Formation in its Wake
DOI: 10.3847/2041-8213/acba86 Bibcode: 2023ApJ...946L..50V

van den Bosch, Frank C.; van Dokkum, Pieter; Romanowsky, Aaron J. +13 more

The interaction of a runaway supermassive black hole (SMBH) with the circumgalactic medium (CGM) can lead to the formation of a wake of shocked gas and young stars behind it. Here we report the serendipitous discovery of an extremely narrow linear feature in Hubble Space Telescope (HST) Advanced Camera for Surveys images that may be an example of …

2023 The Astrophysical Journal
eHST 18
A Near-infrared-faint, Far-infrared-luminous Dusty Galaxy at z ∼ 5 in COSMOS-Web
DOI: 10.3847/1538-4357/acf614 Bibcode: 2023ApJ...956...72M

Casey, Caitlin M.; Kartaltepe, Jeyhan S.; Koekemoer, Anton M. +32 more

A growing number of far-infrared (FIR) bright sources completely invisible in deep extragalactic optical surveys hint at an elusive population of z > 4 dusty, star-forming galaxies. Cycle 1 JWST surveys are now detecting their rest-frame optical light, which provides key insight into their stellar properties and statistical constraints on the p…

2023 The Astrophysical Journal
JWST 18
New Chondritic Bodies Identified in Eight Oxygen-bearing White Dwarfs
DOI: 10.3847/1538-4357/acbd44 Bibcode: 2023ApJ...950...93D

Weinberger, Alycia J.; Zuckerman, B.; Dufour, Patrick +8 more

We present observations and analyses of eight white dwarf stars (WDs) that have accreted rocky material from their surrounding planetary systems. The spectra of these helium-atmosphere WDs contain detectable optical lines of all four major rock-forming elements (O, Mg, Si, and Fe). This work increases the sample of oxygen-bearing WDs with parent b…

2023 The Astrophysical Journal
Gaia 18
Extragalactic Magnetism with SOFIA (SALSA Legacy Program): The Magnetic Fields in the Multiphase Interstellar Medium of the Antennae Galaxies
DOI: 10.3847/2041-8213/acaaa2 Bibcode: 2023ApJ...942L..13L

Reach, William T.; Dale, Daniel A.; Lopez-Rodriguez, Enrique +8 more

Mergers are thought to be a fundamental channel for galaxy growth, perturbing the gas dynamics and the magnetic fields (B-fields) in the interstellar medium (ISM). However, the mechanisms that amplify and dissipate B-fields during a merger remain unclear. We characterize the morphology of the ordered B-fields in the multiphase ISM of the closest m…

2023 The Astrophysical Journal
Herschel eHST 18
CEERS Key Paper. VII. JWST/MIRI Reveals a Faint Population of Galaxies at Cosmic Noon Unseen by Spitzer
DOI: 10.3847/2041-8213/ad0b14 Bibcode: 2023ApJ...959L...7K

Papovich, Casey; Yang, Guang; Finkelstein, Steven L. +33 more

The Cosmic Evolution Early Release Science program observed the Extended Groth Strip (EGS) with the Mid-Infrared Instrument (MIRI) on the James Webb Space Telescope (JWST) in 2022. In this paper, we discuss the four MIRI pointings that observed with longer-wavelength filters, including F770W, F1000W, F1280W, F1500W, F1800W, and F2100W. We compare …

2023 The Astrophysical Journal
JWST 18
Spatial and Temporal Analysis of Quiescent Coronal Rain over an Active Region
DOI: 10.3847/1538-4357/acd44b Bibcode: 2023ApJ...950..171S

Antolin, Patrick; Schad, Thomas A.; Froment, Clara +1 more

The solar corona produces coronal rain, hundreds of times colder and denser material than the surroundings. Coronal rain is known to be deeply linked to coronal heating, but its origin, dynamics, and morphology are still not well understood. The leading theory for its origin is thermal instability (TI) occurring in coronal loops in a state of ther…

2023 The Astrophysical Journal
IRIS 18
Models of Rotating Infall for the B335 Protostar
DOI: 10.3847/1538-4357/acaa38 Bibcode: 2023ApJ...943...90E

Choi, Minho; Di Francesco, James; Lee, Jeong-Eun +7 more

Models of the protostellar source, B335, are developed using axisymmetric three-dimensional models to resolve conflicts found in one-dimensional models. The models are constrained by a large number of observations, including ALMA, Herschel, and Spitzer data. Observations of the protostellar source B335 with ALMA show redshifted absorption against …

2023 The Astrophysical Journal
Gaia Herschel 18
The R-Process Alliance: Chemodynamically Tagged Groups. II. An Extended Sample of Halo r-process-enhanced Stars
DOI: 10.3847/1538-4357/aca322 Bibcode: 2023ApJ...943...23S

Beers, Timothy C.; Placco, Vinicius M.; Holmbeck, Erika M. +8 more

Orbital characteristics based on Gaia Early Data Release 3 astrometric parameters are analyzed for ~1700 r-process-enhanced (RPE; [Eu/Fe] > +0.3) metal-poor stars ([Fe/H] ≤ -0.8) compiled from the R-Process Alliance, the GALactic Archaeology with HERMES (GALAH) DR3 survey, and additional literature sources. We find dynamical clusters of these s…

2023 The Astrophysical Journal
Gaia 18
Metal-enriched Neutral Gas Reservoir around a Strongly Lensed Low-mass Galaxy at z = 4 Identified by JWST/NIRISS and VLT/MUSE
DOI: 10.3847/2041-8213/aca1c4 Bibcode: 2023ApJ...944L..59L

Chevallard, Jacopo; Fan, Xiaohui; Schaerer, Daniel +19 more

Direct observations of low-mass, low-metallicity galaxies at z ≳ 4 provide an indispensable opportunity for detailed inspection of the ionization radiation, gas flow, and metal enrichment in sources similar to those that reionized the universe. Combining the James Webb Space Telescope (JWST), Very Large Telescope/MUSE, and Atacama Large Millimeter…

2023 The Astrophysical Journal
eHST JWST 18