Search Publications

Millisecond Pulsars in Dense Star Clusters: Evolution, Scaling Relations, and the Galactic-center Gamma-Ray Excess
DOI: 10.3847/1538-4357/ac9cd0 Bibcode: 2022ApJ...940..162Y

Ye, Claire S.; Fragione, Giacomo

The number of millisecond pulsars (MSPs) observed in Milky Way globular clusters has increased explosively in recent years, but the underlying population is still uncertain due to observational biases. We use state-of-the-art N-body simulations to study the evolution of MSP populations in dense star clusters. These cluster models span a wide range…

2022 The Astrophysical Journal
Gaia 5
The Effect of Molecular Cloud Properties on the Kinematics of Stars Formed in the Trifid Region
DOI: 10.3847/1538-4357/ac6fe8 Bibcode: 2022ApJ...937...46K

Gromadzki, Mariusz; Feigelson, Eric D.; Hillenbrand, Lynne A. +5 more

The dynamical states of molecular clouds may affect the properties of the stars they form. In the vicinity of the Trifid Nebula (d = 1180 ± 25 pc), the main star cluster (Trifid Main) lies within an expanding section of the molecular cloud; however, ~0.°3 to the north (Trifid North), the cloud's velocity structure is more tranquil. We acquired a C…

2022 The Astrophysical Journal
Gaia 5
Chandra Observations of Six Peter Pan Disks: Diversity of X-Ray-driven Internal Photoevaporation Rates Does Not Explain Their Rare Longevity
DOI: 10.3847/1538-4357/ac8156 Bibcode: 2022ApJ...935..111L

Kounkel, Marina; Kuchner, Marc J.; Wisniewski, John P. +6 more

We present Chandra X-ray observations of six previously identified Peter Pan objects, rare ∼40 Myr systems with evidence of primordial disk retention. We observe X-ray luminosities (0.8–3.0 keV) ranging from log L x ∼ 27.7–29.1. We find that our Peter Pan sample exhibits X-ray properties similar to that of weak-lined T Tauri stars and…

2022 The Astrophysical Journal
Gaia XMM-Newton 5
Spatial Structures in the Globular Cluster Distribution of Fornax Cluster Galaxies
DOI: 10.3847/1538-4357/ac4be2 Bibcode: 2022ApJ...927...15D

Zezas, Andreas; Fabbiano, Giuseppina; Paolillo, Maurizio +3 more

We report the discovery of statistically significant spatial structures in the projected two-dimensional distributions of Globular Cluster (GC) systems of 10 galaxies that are among the brightest in the Fornax Cluster. We use a catalog of GCs extracted from the Hubble Space Telescope Advanced Camera for Surveys Fornax Cluster Survey imaging data. …

2022 The Astrophysical Journal
eHST 5
A Comprehensive Study of the Young Cluster IRAS 05100+3723: Properties, Surrounding Interstellar Matter, and Associated Star Formation
DOI: 10.3847/1538-4357/ac3a78 Bibcode: 2022ApJ...926...16Y

Zavagno, A.; Samal, M. R.; Ojha, D. K. +13 more

We present a comprehensive multiwavelength investigation of a likely massive young cluster "IRAS 05100+3723" and its environment with the aim to understand its formation history and feedback effects. We find that IRAS 05100+3723 is a distant (~3.2 kpc), moderate-mass (~500 M ), young (~3 Myr) cluster with its most massive star being an…

2022 The Astrophysical Journal
Gaia Herschel 4
The Magnetic Field Environment of Active Region 12673 That Produced the Energetic Particle Events of September 2017
DOI: 10.3847/1538-4357/ac8d69 Bibcode: 2022ApJ...937...57Y

Green, Lucie M.; Yardley, Stephanie L.; Mihailescu, Teodora +2 more

Forecasting solar energetic particles (SEPs), and identifying flares/coronal mass ejections (CMEs) from active regions (ARs) that will produce SEP events in advance is extremely challenging. We investigate the magnetic field environment of AR 12673, including the AR's magnetic configuration, the surrounding field configuration in the vicinity of t…

2022 The Astrophysical Journal
SOHO 4
Morpho-kinematic Modeling of the Expanding Ejecta of the Extremely Slow Nova V1280 Scorpii
DOI: 10.3847/1538-4357/ac6c82 Bibcode: 2022ApJ...932...39N

Maehara, Hiroyuki; Sakon, Itsuki; Watanabe, Makoto +10 more

Knowledge of the morphology of nova ejecta is essential for fully understanding the physical processes involved in nova eruptions. We studied the 3D morphology of the expanding ejecta of the extremely slow nova V1280 Sco with a unique light curve. Synthetic line profile spectra were compared to the observed [O III] λλ4959, 5007 and [N II] λ5755 em…

2022 The Astrophysical Journal
Gaia 4
Density Turbulence and the Angular Broadening of Outer Heliospheric Radio Sources at High Latitudes and in the Ecliptic Plane
DOI: 10.3847/1538-4357/ac5031 Bibcode: 2022ApJ...928..125T

Cairns, Iver H.; Adhikari, L.; Tasnim, Samira +1 more

Density irregularities are responsible for the scattering of radio waves in the solar wind and astrophysical plasmas. These irregularities significantly affect the inferred physical properties of radio sources, such as size, direction, and intensity. We present here a theory of angular broadening due to the scattering of radio waves by density irr…

2022 The Astrophysical Journal
Ulysses 4
Widespread 1-2 MeV Energetic Particles Associated with Slow and Narrow Coronal Mass Ejections: Parker Solar Probe and STEREO Measurements
DOI: 10.3847/1538-4357/ac3af2 Bibcode: 2022ApJ...925...96Z

Lugaz, Noé; Zhuang, Bin; Lario, David

Suprathermal ions in the corona are thought to serve as seed particles for large gradual solar energetic particle (SEP) events associated with fast and wide coronal mass ejections (CMEs). A better understanding of the role of suprathermal particles as seed populations for SEP events can be made by using observations close to the Sun. We study a se…

2022 The Astrophysical Journal
SOHO 4
Polarization Spectrum of Near-Infrared Zodiacal Light Observed with CIBER
DOI: 10.3847/1538-4357/ac416f Bibcode: 2022ApJ...926....6T

Shirahata, Mai; Cooray, Asantha; Matsuura, Shuji +14 more

We report the first measurement of the zodiacal light (ZL) polarization spectrum in the near-infrared between 0.8 and 1.8 µm. Using the low-resolution spectrometer on board the Cosmic Infrared Background Experiment, calibrated for absolute spectrophotometry and spectropolarimetry, we acquire long-slit polarization spectral images of the tota…

2022 The Astrophysical Journal
AKARI 4