Search Publications

A Tale of Three Dwarfs: Cluster-based Star Formation Histories of Blue Compact Dwarf Galaxies
DOI: 10.3847/1538-4357/ad293a Bibcode: 2024ApJ...965...95C

Calzetti, Daniela; Whitmore, Bradley C.; Chandar, Rupali +9 more

We present a new study of the cluster populations in the blue compact dwarf galaxies (BCD) ESO185-IG13, ESO338-IG04, and Haro11, based on new and archival high-resolution images taken by the Hubble Space Telescope, and the first to probe the populations older than ≈100 Myr. BCDs are believed to experience intense bursts of star formation (includin…

2024 The Astrophysical Journal
eHST 0
Temperature Intermittent Structures in the Fast Solar Wind
DOI: 10.3847/1538-4357/ad3239 Bibcode: 2024ApJ...966..153W

Wang, Xin; Wang, Yuxin; Song, Dongze +1 more

In the solar wind turbulence, proton temperature fluctuations are highly intermittent, especially at small scales in the inertial range. This phenomenon may contain information about solar wind intermittent heating. However, the physical nature of the temperature intermittency is not yet clear. Based on the measurements from Solar Orbiter between …

2024 The Astrophysical Journal
SolarOrbiter 0
Electron Densities of Transition Region Loops Derived from IRIS O IV Spectral Data
DOI: 10.3847/2041-8213/ad3d5e Bibcode: 2024ApJ...966L...6L

Fu, Hui; Xia, Lidong; Huang, Zhenghua +4 more

Loops are fundamental structures in the magnetized atmosphere of the Sun. Their physical properties are crucial for understanding the nature of the solar atmosphere. Transition region loops are relatively dynamic and their physical properties have not yet been fully understood. With spectral data of the line pair of O IV 1399.8 Å and 1401.2 Å (

2024 The Astrophysical Journal
IRIS 0
Aperture and Resolution Effects on Ultraviolet Star-forming Properties: Insights from Local Galaxies and Implications for High-redshift Observations
DOI: 10.3847/1538-4357/ad1dde Bibcode: 2024ApJ...964...25C

Leitherer, Claus; Berg, Danielle A.; Arellano-Córdova, Karla Z. +2 more

We present an analysis of the effects of spectral resolution and aperture scale on derived galaxy properties using far-ultraviolet (FUV) spectra of local star-forming galaxies from the International Ultraviolet Explorer (R ∼ 250, field of view (FOV) ∼ 10″ × 20″) and Cosmic Origins Spectrograph on the Hubble Space Telescope (R ∼ 15,000, FOV ∼ 2.″5)…

2024 The Astrophysical Journal
IUE eHST 0
The Relative Prevalence of Wave Packets and Coherent Structures in the Inertial and Kinetic Ranges of Turbulence as Seen by Solar Orbiter
DOI: 10.3847/1538-4357/ad54bc Bibcode: 2024ApJ...971..179B

Dudok de Wit, Thierry; Bendt, Alina; Chapman, Sandra

The Solar Orbiter (SO) mission provides the opportunity to study the evolution of solar wind turbulence. We use SO observations of nine extended intervals of homogeneous turbulence to determine when turbulent magnetic field fluctuations may be characterized as: (i) wave packets and (ii) coherent structures (CSs). We perform the first systematic sc…

2024 The Astrophysical Journal
SolarOrbiter 0
JWST Reveals Bulge-dominated Star-forming Galaxies at Cosmic Noon
DOI: 10.3847/2041-8213/ad7e27 Bibcode: 2024ApJ...974L..28B

van Dokkum, Pieter; van der Wel, Arjen; Bezanson, Rachel +10 more

Hubble Space Telescope imaging shows that most star-forming galaxies at cosmic noon—the peak of cosmic star formation history—appear disk-dominated, leaving the origin of the dense cores in their quiescent descendants unclear. With the James Webb Space Telescope's high-resolution imaging to 5 µm, we can now map the rest-frame near-infrared e…

2024 The Astrophysical Journal
eHST JWST 0
2FHL J1745.1–3035: A Newly Discovered, Powerful Pulsar Wind Nebula Candidate
DOI: 10.3847/1538-4357/ad2614 Bibcode: 2024ApJ...964..132M

Vignali, C.; Ajello, M.; Tibaldo, L. +8 more

We present a multi-epoch, multi-observatory X-ray analysis for 2FHL J1745.1–3035, a newly discovered very high-energy Galactic source detected by the Fermi Large Area Telescope (LAT) located in close proximity to the Galactic Center (l = 358.°5319; b = ‑0.°7760). The source shows a very hard γ-ray photon index above 50 GeV, Γ γ = 1.2 ±…

2024 The Astrophysical Journal
Gaia XMM-Newton 0
A Precursor to Solar Prominence Eruptions: Detection and Analysis of EUV Prominence Oscillations
DOI: 10.3847/1538-4357/ad8e3c Bibcode: 2024ApJ...977..253B

Foullon, Claire; Verwichte, Erwin; Beckwith-Chandler, William

The eruption of prominences can have a significant influence on the solar–terrestrial environment. However, accurately predicting these eruptions remains a challenge. We apply automated detection methods for extreme ultraviolet (EUV) prominences observed by the twin spacecraft from the Solar Terrestrial Relations Observatory (STEREO) mission and t…

2024 The Astrophysical Journal
SOHO 0
The Differences in the Origination and Properties of the Near-Earth Solar Wind between Solar Cycles 23 and 24
DOI: 10.3847/1538-4357/ad5be1 Bibcode: 2024ApJ...972...54S

Fu, Hui; Xia, Lidong; Huang, Zhenghua +5 more

The dependence of the sources and properties of the near-Earth solar wind on solar cycle activity is an important issue in solar and space physics. We use the improved "two-step" mapping procedure that takes into account the initial acceleration processes to trace the near-Earth solar winds back to their source regions from 1999–2020, covering sol…

2024 The Astrophysical Journal
SOHO 0
Visit Nearby Halo Substructures Using LAMOST DR9 MRS Data
DOI: 10.3847/1538-4357/ad3240 Bibcode: 2024ApJ...965...62T

Zhao, Gang; Zhao, Jing-Kun; Gao, Qi +3 more

Based on the LAMOST DR9 Medium Resolution Spectra (MRS) catalog, combined with astrometries from Gaia DR3, we conducted an investigation into the substructures in the stellar halo to obtain their chemical and kinematic information. We employed the HDBSCAN algorithm in the (L z , E, L xy ) space for clustering and utilized M…

2024 The Astrophysical Journal
Gaia 0