Search Publications

Parallel Diffusion Coefficient of Energetic Charged Particles in the Inner Heliosphere from the Turbulent Magnetic Fields Measured by Parker Solar Probe
DOI: 10.3847/1538-4357/ad33c3 Bibcode: 2024ApJ...965...61C

Klein, Kristopher G.; Chen, Xiaohang; Giacalone, Joe +1 more

Diffusion coefficients of energetic charged particles in turbulent magnetic fields are a fundamental aspect of diffusive transport theory but remain incompletely understood. In this work, we use quasi-linear theory to evaluate the spatial variation of the parallel diffusion coefficient κ from the measured magnetic turbulence power spe…

2024 The Astrophysical Journal
Ulysses 6
Tracing the Origins of Mass Segregation in M35: Evidence for Primordially Segregated Binaries
DOI: 10.3847/2041-8213/ad18bf Bibcode: 2024ApJ...962L...9M

von Hippel, Ted; Motherway, Erin; Geller, Aaron M. +2 more

M35 is a young open cluster and home to an extensive binary population. Using Gaia Data Release 3, Pan-STARRS, and Two Micron All Sky Survey photometry with the Bayesian statistical software, BASE-9, we derive precise cluster parameters, identify single and binary cluster members, and extract their masses. We identify 571 binaries down to Gaia G =…

2024 The Astrophysical Journal
Gaia 6
The Effect of Starspots on Spectroscopic Age and Mass Estimates of Nonaccreting T Tauri Stars in the Taurus–Auriga Star-forming Region
DOI: 10.3847/1538-4357/ad393b Bibcode: 2024ApJ...967...45P

Hillenbrand, Lynne A.; Markham, Madison; Bary, Jeffrey S. +1 more

Accurate age and mass determinations for young pre-main-sequence stars are made challenging by the presence of large-scale starspots. We present results from a near-infrared spectroscopic survey of 10 T-Tauri Stars in Taurus-Auriga that characterize spot-filling factors and temperatures, the resulting effects on temperature and luminosity determin…

2024 The Astrophysical Journal
Gaia 6
The Orbit and Dynamical Mass of Polaris: Observations with the CHARA Array
DOI: 10.3847/1538-4357/ad5e7a Bibcode: 2024ApJ...971..190E

Torres, Guillermo; Mérand, Antoine; Monnier, John D. +19 more

The 30 yr orbit of the Cepheid Polaris has been followed with observations by the Center for High Angular Resolution Astronomy (CHARA) Array from 2016 through 2021. An additional measurement has been made with speckle interferometry at the Apache Point Observatory. Detection of the companion is complicated by its comparative faintness—an extreme f…

2024 The Astrophysical Journal
Gaia eHST 6
AGN STORM 2. VII. A Frequency-resolved Map of the Accretion Disk in Mrk 817: Simultaneous X-Ray Reverberation and UVOIR Disk Reprocessing Time Lags
DOI: 10.3847/1538-4357/ad6b08 Bibcode: 2024ApJ...974..271L

Kaspi, Shai; Barth, Aaron J.; Horne, Keith +35 more

X-ray reverberation mapping is a powerful technique for probing the innermost accretion disk, whereas continuum reverberation mapping in the UV, optical, and infrared (UVOIR) reveals reprocessing by the rest of the accretion disk and broad-line region (BLR). We present the time lags of Mrk 817 as a function of temporal frequency measured from 14 m…

2024 The Astrophysical Journal
XMM-Newton 6
The Factory and the Beehive. V. Chromospheric and Coronal Activity and Its Dependence on Rotation in Praesepe and the Hyades
DOI: 10.3847/1538-4357/ad117e Bibcode: 2024ApJ...962...12N

Drake, Jeremy J.; Covey, Kevin R.; Agüeros, Marcel A. +6 more

Low-mass (≲1.2 M ) main-sequence stars lose angular momentum over time, leading to a decrease in their magnetic activity. The details of this rotation–activity relation remain poorly understood, however. Using observations of members of the ≈700 Myr old Praesepe and Hyades open clusters, we aim to characterize the rotation–activity rel…

2024 The Astrophysical Journal
Gaia XMM-Newton 6
Why Are (Almost) All the Protostellar Outflows Aligned in Serpens Main?
DOI: 10.3847/1538-4357/ad5a02 Bibcode: 2024ApJ...972....5G

Manoj, P.; Narang, Mayank; Reiter, Megan +4 more

We present deep 1.4–4.8 µm JWST-NIRCam imaging of the Serpens Main star-forming region and identify 20 candidate protostellar outflows, most with bipolar structure and identified driving sources. The outflow position angles (PAs) are strongly correlated, and they are aligned within ±24° of the major axis of the Serpens filament. These orient…

2024 The Astrophysical Journal
JWST 5
JWST's First Glimpse of a z > 2 Forming Cluster Reveals a Top-heavy Stellar Mass Function
DOI: 10.3847/2041-8213/ad4986 Bibcode: 2024ApJ...967L..34S

Daddi, Emanuele; Lu, Shiying; Kodama, Tadayuki +11 more

Clusters and their progenitors (protoclusters) at z ∼ 2 ‑ 4, the peak epoch of star formation, are ideal laboratories to study the formation process of both the clusters themselves and their member galaxies. However, a complete census of their member galaxies has been challenging due to observational difficulties. Here we present new JWST/NIRCam o…

2024 The Astrophysical Journal
eHST JWST 5
Solar Eruptions in Nested Magnetic Flux Systems
DOI: 10.3847/1538-4357/ad2eaa Bibcode: 2024ApJ...966...27K

Antiochos, Spiro K.; Kumar, Pankaj; DeVore, C. Richard +2 more

The magnetic topology of erupting regions on the Sun is a key factor in the energy buildup and release, and the subsequent evolution of flares and coronal mass ejections (CMEs). The presence/absence of null points and separatrices dictates whether and where current sheets form and magnetic reconnection occurs. Numerical simulations show that energ…

2024 The Astrophysical Journal
SOHO 5
The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems. IV. NIRISS Aperture Masking Interferometry Performance and Lessons Learned
DOI: 10.3847/2041-8213/ad21fb Bibcode: 2024ApJ...963L...2S

Henning, Thomas; Fortney, Jonathan J.; Moran, Sarah E. +120 more

We present a performance analysis for the aperture masking interferometry (AMI) mode on board the James Webb Space Telescope Near Infrared Imager and Slitless Spectrograph (JWST/NIRISS). Thanks to self-calibrating observables, AMI accesses inner working angles down to and even within the classical diffraction limit. The scientific potential of thi…

2024 The Astrophysical Journal
JWST 5