Search Publications

A Study of Stellar Spins in 15 Open Clusters
DOI: 10.3847/1538-4357/acad7b Bibcode: 2023ApJ...944...39H

Schlaufman, Kevin C.; Healy, Brian F.; McCullough, P. R. +1 more

We analyze spectroscopic and photometric data to determine the projected inclinations of stars in 11 open clusters, placing constraints on the spin-axis distributions of six clusters. We combine these results with four additional clusters studied by Healy & McCullough and Healy et al. to perform an ensemble analysis of their spins. We find tha…

2023 The Astrophysical Journal
Gaia 9
The Evaporating Massive Embedded Stellar Cluster IRS 13 Close to Sgr A*. I. Detection of a Rich Population of Dusty Objects in the IRS 13 Cluster
DOI: 10.3847/1538-4357/acf6b5 Bibcode: 2023ApJ...956...70P

Eckart, Andreas; Zajaček, Michal; Labadie, Lucas +6 more

A detailed analysis of the nuclear star cluster not only concedes the existence of the S cluster, with its fast-moving stars and the supermassive black hole Sgr A*. It also reveals an embedded region of gas and dust with an exceptionally high stellar density called IRS 13. The IRS 13 cluster can be divided into the northern and eastern counterpart…

2023 The Astrophysical Journal
JWST 9
ALMA Measurement of 10 kpc Scale Lensing-power Spectra toward the Lensed Quasar MG J0414+0534
DOI: 10.3847/1538-4357/aceb5f Bibcode: 2023ApJ...954..197I

Matsushita, Satoki; Minezaki, Takeo; Nakanishi, Kouichiro +1 more

The lensing power spectra for gravitational potential, astrometric shift, and convergence perturbations are powerful probes to investigate dark matter structures on small scales. We report the first lower and upper bounds of these lensing power spectra on angular scale ~1″ toward the anomalous quadruply lensed quasar MG J0414+0534 at a redshift z …

2023 The Astrophysical Journal
eHST 9
Implications of Different Solar Photospheric Flux-transport Models for Global Coronal and Heliospheric Modeling
DOI: 10.3847/1538-4357/acba8e Bibcode: 2023ApJ...946..105B

Cheung, Mark C. M.; DeRosa, Marc L.; Barnes, Graham +3 more

The concept of surface-flux transport (SFT) is commonly used in evolving models of the large-scale solar surface magnetic field. These photospheric models are used to determine the large-scale structure of the overlying coronal magnetic field, as well as to make predictions about the fields and flows that structure the solar wind. We compare predi…

2023 The Astrophysical Journal
SOHO 9
First Results from the JWST Early Release Science Program Q3D: Benchmark Comparison of Optical and Mid-infrared Tracers of a Dusty, Ionized Red Quasar Wind at z = 0.435
DOI: 10.3847/2041-8213/aced85 Bibcode: 2023ApJ...953L..26R

Shen, Lu; Johnson, Sean D.; Lützgendorf, Nora +27 more

The [O III] 5007 Å emission line is the most common tracer of warm, ionized outflows in active galactic nuclei across cosmic time. JWST newly allows us to use mid-IR spectral features at both high spatial and spectral resolution to probe these same winds. Here we present a comparison of ground-based, seeing-limited [O III] and space-based, diffrac…

2023 The Astrophysical Journal
JWST 9
Lyα Scattering Models Trace Accretion and Outflow Kinematics in T Tauri Systems
DOI: 10.3847/1538-4357/acaf70 Bibcode: 2023ApJ...944..185A

Herczeg, Gregory J.; France, Kevin; Ábrahám, Péter +18 more

T Tauri stars produce broad Lyα emission lines that contribute ~88% of the total UV flux incident on the inner circumstellar disks. Lyα photons are generated at the accretion shocks and in the protostellar chromospheres and must travel through accretion flows, winds, and jets, the protoplanetary disks, and the interstellar medium before reaching t…

2023 The Astrophysical Journal
Herschel eHST 9
Pixelated Reconstruction of Foreground Density and Background Surface Brightness in Gravitational Lensing Systems Using Recurrent Inference Machines
DOI: 10.3847/1538-4357/accf84 Bibcode: 2023ApJ...951....6A

Hezaveh, Yashar; Adam, Alexandre; Perreault-Levasseur, Laurence +1 more

Modeling strong gravitational lenses in order to quantify distortions in the images of background sources and to reconstruct the mass density in foreground lenses has been a difficult computational challenge. As the quality of gravitational lens images increases, the task of fully exploiting the information they contain becomes computationally and…

2023 The Astrophysical Journal
eHST 9
A Large-scale Kinematic Study of Molecular Gas in High-z Cluster Galaxies: Evidence for High Levels of Kinematic Asymmetry
DOI: 10.3847/1538-4357/acae96 Bibcode: 2023ApJ...944..213C

Cooper, M. C.; Clements, D. L.; van Kampen, E. +14 more

We investigate the resolved kinematics of the molecular gas, as traced by the Atacama Large Millimeter/submillimeter Array in CO (2-1), of 25 cluster member galaxies across three different clusters at a redshift of z ~ 1.6. This is the first large-scale analysis of the molecular gas kinematics of cluster galaxies at this redshift. By separately es…

2023 The Astrophysical Journal
eHST 9
The Close AGN Reference Survey (CARS): An Interplay between Radio Jets and AGN Radiation in the Radio-quiet AGN HE0040-1105
DOI: 10.3847/1538-4357/ad004d Bibcode: 2023ApJ...959..107S

Gaspari, M.; Combes, F.; O'Dea, C. P. +14 more

We present a case study of HE 0040-1105, an unobscured radio-quiet active galactic nucleus (AGN) at a high accretion rate of λ Edd = 0.19 ± 0.04. This particular AGN hosts an ionized gas outflow with the largest spatial offset from its nucleus compared to all other AGNs in the Close AGN Reference Survey. By combining multiwavelength obs…

2023 The Astrophysical Journal
eHST 9
The Space Weather Context of the First Extreme Event of Solar Cycle 25, on 2022 September 5
DOI: 10.3847/1538-4357/acf30f Bibcode: 2023ApJ...956...58P

Vourlidas, Angelos; Kouloumvakos, Athanasios; Papaioannou, Athanasios +3 more

The coronal mass ejection (CME) on 2022 September 5 was the fastest CME yet observed and measured in situ by a spacecraft inside the corona (0.06 au for the Parker Solar Probe). Here we assess the significance of this event for space weather studies by analyzing the source region characteristics and its temporal evolution via a magnetic complexity…

2023 The Astrophysical Journal
SolarOrbiter 9