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The Astrophysical Journal (ApJ)

Resumen/Descripción – provisto por la editorial en inglés
The Astrophysical Journal is an open access journal devoted to recent developments, discoveries, and theories in astronomy and astrophysics. Publications in ApJ constitute significant new research that is directly relevant to astrophysical applications, whether based on observational results or on theoretical insights or modeling.
Palabras clave – provistas por la editorial

astronomy; astrophysics

Disponibilidad
Institución detectada Período Navegá Descargá Solicitá
No detectada desde jul. 1995 / hasta dic. 2023 IOPScience

Información

Tipo de recurso:

revistas

ISSN impreso

0004-637X

ISSN electrónico

1538-4357

Editor responsable

American Astronomical Society (AAS)

Idiomas de la publicación

  • inglés

País de edición

Reino Unido

Información sobre licencias CC

https://creativecommons.org/licenses/by/4.0/

Cobertura temática

Tabla de contenidos

Self-consistent 3D Supernova Models From −7 Minutes to +7 s: A 1-bethe Explosion of a ∼19 M Progenitor

Robert BolligORCID; Naveen YadavORCID; Daniel KresseORCID; Hans-Thomas JankaORCID; Bernhard MüllerORCID; Alexander HegerORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 28

Trajectory Analysis of Galactic Cosmic Rays Invading into the Heliosphere

Kotaro YoshidaORCID; Shuichi MatsukiyoORCID; Kesuke Shimokawa; Haruichi Washimi; Tohru HadaORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 29

Sensitivity Study of r-process Abundances to Nuclear Masses

X. F. Jiang; X. H. Wu; P. W. Zhao

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 29

Linear and Nonlinear Effects of Proton Temperature Anisotropy on Proton-beam Instability in the Solar Wind

L. Xiang; K. H. Lee; D. J. WuORCID; H. W. Yu; L. C. LeeORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 30

Numerical Research on the Effect of the Initial Parameters of a CME Flux-rope Model on Simulation Results. II. Different Locations of Observers

Fang ShenORCID; Yousheng Liu; Yi Yang

<jats:title>Abstract</jats:title> <jats:p>In numerical studies of the initiation and propagation of coronal mass ejections (CMEs), it has been proven that the shape, size, and plasma parameters of CMEs could significantly affect simulation results and subsequent space weather predictions. In our previous research, we proposed a new way to initiate a CME based on the graduated cylindrical shell model, and studied the effect of different initial parameters of CMEs on the simulation results when the observer is aligned with the initial propagation direction of the CME. In this paper, we investigate the influence of the different initial parameters of CMEs on simulation results at the observational points with different longitudes and latitudes. Our results indicate that as long as the initial mass of the CME remains unchanged, the initial geometric thickness will have a different influence in the latitudinal and longitudinal directions. The deflection of the CMEs always occurs in both latitudinal and longitudinal directions, when the CMEs interact with the background solar wind structures, such as the corotating interaction region, in the heliosphere.</jats:p>

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 30

Radiative Driving of the AGN Outflows in the Narrow-line Seyfert 1 Galaxy NGC 4051* †

Beena MeenaORCID; D. Michael CrenshawORCID; Henrique R. SchmittORCID; Mitchell RevalskiORCID; Travis C. FischerORCID; Garrett E. PolackORCID; Steven B. KraemerORCID; Dzhuliya DashtamirovaORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 31

Magnetically Arrested Disks in Quiescent Black Hole Binaries: Formation Scenario, Observable Signatures, and Potential PeVatrons

Shigeo S. KimuraORCID; Takahiro SudohORCID; Kazumi KashiyamaORCID; Norita KawanakaORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 31

X-Ray Superflares from Pre-main-sequence Stars: Flare Energetics and Frequency

Konstantin V. GetmanORCID; Eric D. FeigelsonORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 32

Spectroscopic Confirmation of Two Extremely Massive Protoclusters, BOSS1244 and BOSS1542, at z = 2.24

Dong Dong ShiORCID; Zheng CaiORCID; Xiaohui FanORCID; Xian Zhong ZhengORCID; Yun-Hsin HuangORCID; Jiachuan Xu

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 32

Milky Way Mid-Infrared Spitzer Spectroscopic Extinction Curves: Continuum and Silicate Features

Karl D. GordonORCID; Karl A. Misselt; Jeroen BouwmanORCID; Geoffrey C. ClaytonORCID; Marjorie DecleirORCID; Dean C. HinesORCID; Yvonne PendletonORCID; George RiekeORCID; J. D. T. SmithORCID; D. C. B. WhittetORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. 33