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Quadrupole White-light Sources in an X1.2 Flare Observed by ASO-S/LST/WST and SDO/HMI

Zhichen Jing, Ying Li, Dechao Song, Qiao Li et al. • The Astrophysical Journal (2026)

We present observations of an X1.2 white-light flare on 2023 January 6, which exhibits a rare quadrupolar white-light source configuration. This event was observed by the White-light Solar Telescope (WST; 3600 Å) onboard the Advanced Space-...

DOAJ Open Access (DOAJ) DOI: 10.3847/1538-4357/ae9161

Tera-Hertz Counterparts to Fast Radio Bursts from Coherent Cherenkov Radiation by Tilted Bunches

Ze-Nan Liu, Wei-Yang Wang, Yu-Chen Huang, Zi-Gao Dai • The Astrophysical Journal (2025)

Fast radio bursts (FRBs) are millisecond-duration extragalactic transients characterized by ultrahigh brightness temperatures, suggesting coherent emission mechanisms in extreme astrophysical processes. In this paper, we extend the bunched ...

DOAJ Open Access (DOAJ) DOI: 10.3847/1538-4357/adea76

Physical Characterization of Early Galaxies in the Webb’s First Deep Field SMACS J0723.3-7327

T. Morishita, M. Stiavelli • The Astrophysical Journal Letters (2023)

This paper highlights initial photometric analyses of JWST NIRCam imaging data in the sightline of SMACS0723, aiming to identify galaxies at redshift z > 7. By applying a conservative Lyman-break selection followed by photometric-redshift a...

DOAJ Open Access (DOAJ) DOI: 10.3847/2041-8213/acbf50

Investigating the Impact of Supernova Feedback on Satellites in Elliptical Galaxies

Sumi Kim, Ena Choi, Amanda C. N. Quirk, Rachel S. Somerville et al. • The Astrophysical Journal (2025)

We investigate the influence of supernova (SN) feedback on the satellites of elliptical host galaxies using hydrodynamic simulations. Utilizing a modified version of the GADGET-3 code, we perform cosmological zoom-in simulations of 11 ellip...

DOAJ Open Access (DOAJ) DOI: 10.3847/1538-4357/adec96

A tetraquark 81-plet with $$J^{PC}=1^{-+}$$ J PC = 1 - + or a hybrid nonet

Niu Su, Er-Liang Cui, Yi-Wei Jiang, Hua-Xing Chen • European Physical Journal C: Particles and Fields (2026)

Abstract Confirming the existence of hybrid states remains challenging due to their experimental indistinguishability from tightly bound tetraquarks and loosely bound molecules. To address this issue, we employ QCD sum rules to systematical...

DOAJ Open Access (DOAJ) DOI: 10.1140/epjc/s10052-026-15939-y

The Be star o Cas is indeed the primary of a triple system

Harmanec P., Yang S., Šlechta M., Grundstrom E. D. et al. • Astronomy & Astrophysics (2026)

Analysis of radial velocities of two narrow absorption components in the Mg II 4481 Å line demonstrated that the secondary of the Be star o Cas is indeed a close binary system composed of two B7 stars orbiting each other with a period of ...

DOAJ Open Access (DOAJ) DOI: 10.1051/0004-6361/202659678

Investigating the timelike Compton scattering in photon–proton interactions at the EIC

Ya-Ping Xie, V. P. Gonçalves • European Physical Journal C: Particles and Fields (2024)

Abstract Information about the three-dimensional description of the quark and gluon content of hadrons, described by the generalized parton distributions (GPDs), can be probed by exclusive processes in electron–proton (ep) collisions. In th...

DOAJ Open Access (DOAJ) DOI: 10.1140/epjc/s10052-024-13296-2

27 yr of Spaceborne IR Astronomy: An ISO, Spitzer, WISE, and NEOWISE Survey for Large-amplitude Variability in Young Stellar Objects

Chinmay S. Kulkarni, Thomas Behling, Elisabeth E. Banks, Jason Jones et al. • The Astrophysical Journal (2026)

Infrared observations can probe photometric variability across the full evolutionary range of young stellar objects (YSOs), from deeply embedded protostars to pre-main-sequence stars with dusty disks. We present 3–8 μ m light curves extendi...

DOAJ Open Access (DOAJ) DOI: 10.3847/1538-4357/ae3156

FEAST: JWST Uncovers the Emerging Timescales of Young Star Clusters in M83

Alice Knutas, Angela Adamo, Alex Pedrini, Sean T. Linden et al. • The Astrophysical Journal (2025)

We present JWST NIRCam observations of the emerging young star clusters (eYSCs) detected in the nearby spiral galaxy M83. The NIRcam mosaic encompasses the nuclear starburst, the bar, and the inner spiral arms. The eYSCs, detected in Pa α a...

DOAJ Open Access (DOAJ) DOI: 10.3847/1538-4357/ae018c

High-Energy Neutrino Astrophysics

J. G. Learned, Karl Mannheim M • Annual Review of Nuclear and Particle Science (2000)

▪ Abstract High-energy (>100 MeV) neutrino astrophysics enters an era of opportunity and discovery as the sensitivity of detectors approaches astrophysically relevant flux levels. We review the major challenges for this emerging field, amon...

OPENALEX DOI: https://doi.org/10.1146/annurev.nucl.50.1.679

ASTROPHYSICS

Ved Prakash, R Dharanishwari, Jayashree LM, Boya pavani • International Journal of Innovative Research in Information Security (2023)

Astrophysics is a branch of space science that applies the laws of physics and chemistry to seek to understand the universe and our place in it. The field explores topics such as the birth, life and death of stars, planets, galaxies, nebula...

OPENALEX cc-by DOI: https://doi.org/10.26562/ijiris.2023.v0903.09

Astrophysics of Planet Formation

Philip J. Armitage • Cambridge University Press eBooks (2009)

Concise and self-contained, this textbook gives a graduate-level introduction to the physical processes that shape planetary systems, covering all stages of planet formation. Writing for readers with undergraduate backgrounds in physics, as...

OPENALEX Open Access DOI: https://doi.org/10.1017/9781108344227

Advancing Astrophysics with the Square Kilometre Array

Robert L. Braun, Tyler L. Bourke, James Green, Evan Francis Keane et al. • Advancing Astrophysics with the Square Kilometre Array (AASKA) (2015)

In 2014 it was 10 years since the publication of the comprehensive ‘Science with the Square Kilometre Array’ book and 15 years since the first such volume appeared in 1999. In that time numerous and unexpected advances have been made in the...

OPENALEX cc-by-nc-sa DOI: https://doi.org/10.22323/1.215.0174