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The Astrophysical Journal Letters (ApJL)

Resumen/Descripción – provisto por la editorial en inglés
The Astrophysical Journal Letters is an open access express scientific journal that allows astrophysicists to rapidly publish short notices of significant original research. ApJL articles are timely, high-impact, and broadly understandable.
Palabras clave – provistas por la editorial

astronomy; astrophysics

Disponibilidad
Institución detectada Período Navegá Descargá Solicitá
No detectada desde ene. 2010 / hasta dic. 2023 IOPScience

Información

Tipo de recurso:

revistas

ISSN impreso

2041-8205

ISSN electrónico

2041-8213

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

Electromagnetic Precursors to Gravitational-wave Events: Numerical Simulations of Flaring in Pre-merger Binary Neutron Star Magnetospheres

Elias R. MostORCID; Alexander A. PhilippovORCID

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

Pp. L6

First-principles Demonstration of Diffusive-advective Particle Acceleration in Kinetic Simulations of Relativistic Plasma Turbulence

Kai Wong; Vladimir Zhdankin; Dmitri A. Uzdensky; Gregory R. WernerORCID; Mitchell C. BegelmanORCID

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

Pp. L7

The NANOGrav 11 yr Data Set: Constraints on Planetary Masses Around 45 Millisecond Pulsars

E. A. BehrensORCID; S. M. RansomORCID; D. R. MadisonORCID; Z. Arzoumanian; K. Crowter; M. E. DeCesarORCID; P. B. DemorestORCID; T. DolchORCID; J. A. Ellis; R. D. FerdmanORCID; E. C. Ferrara; E. FonsecaORCID; P. A. GentileORCID; G. Jones; M. L. JonesORCID; M. T. LamORCID; L. LevinORCID; D. R. LorimerORCID; R. S. LynchORCID; M. A. McLaughlinORCID; C. NgORCID; D. J. NiceORCID; T. T. PennucciORCID; B. B. P. PereraORCID; P. S. RayORCID; R. SpiewakORCID; I. H. StairsORCID; K. StovallORCID; J. K. SwiggumORCID; W. W. ZhuORCID

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

Pp. L8

The Satellite Luminosity Function of M101 into the Ultra-faint Dwarf Galaxy Regime

P. BennetORCID; D. J. SandORCID; D. CrnojevićORCID; K. SpekkensORCID; A. KarunakaranORCID; D. ZaritskyORCID; B. Mutlu-PakdilORCID

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

Pp. L9

Electron-only Reconnection in Kinetic-Alfvén Turbulence

Cristian Vega; Vadim RoytershteynORCID; Gian Luca Delzanno; Stanislav BoldyrevORCID

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

Pp. L10

Multiple X-line Reconnection Observed in Mercury’s Magnetotail Driven by an Interplanetary Coronal Mass Ejection

J. ZhongORCID; L. C. Lee; X. G. Wang; Z. Y. Pu; J. S. HeORCID; Y. Wei; W. X. Wan

<jats:title>Abstract</jats:title> <jats:p>How magnetic reconnection drives Mercury’s magnetospheric dynamics under extreme solar wind conditions is not well understood. Here we report MESSENGER observations of an active reconnection event in Mercury’s magnetotail driven by an interplanetary coronal mass ejection on 2011 November 23. The primary Hall magnetic field, sequential passage of X-lines with Hall field perturbations, and flux ropes (FRs) provide unambiguous evidence of multiple X-line reconnection in an unstable ion diffusion region. In addition, large FRs consisting of multiple successive small-scale FRs are ejected tailward at quasi-periodic intervals of ∼1 minute, which is comparable to the Dungey cycle time. We propose that these large FRs are generated by the interaction and coalescence of multiple ion-scale FRs. This is distinct from the commonly accepted Earth-like substorm process where plasmoids are created by widely separated X-lines in the magnetotail. These observations suggest that during extreme solar wind conditions multiple X-line reconnection may dominate the tail reconnection process and control the global dynamics of Mercury’s magnetosphere.</jats:p>

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

Pp. L11

Dust Environment Model of the Interstellar Comet 2I/Borisov

G. CremoneseORCID; M. FulleORCID; P. Cambianica; G. Munaretto; M. T. Capria; F. La Forgia; M. Lazzarin; A. Migliorini; W. Boschin; G. Milani; A. Aletti; G. Arlic; P. Bacci; R. Bacci; E. Bryssinck; D. Carosati; D. Castellano; L. Buzzi; S. Di Rubbo; M. Facchini; E. Guido; F. Kugel; R. Ligustri; M. Maestripieri; A. Mantero; J. Nicolas; P. Ochner; C. Perrella; R. Trabatti; A. Valvasori

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

Pp. L12

A White-light Flare Powered by Magnetic Reconnection in the Lower Solar Atmosphere

Yongliang SongORCID; Hui TianORCID; Xiaoshuai Zhu; Yajie Chen; Mei Zhang; Jingwen Zhang

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

Pp. L13

Gamma-Ray Burst Spectrum with a Time-dependent Injection Rate of High-energy Electrons

Kuan Liu; Da-Bin LinORCID; Kai Wang; Li Zhou; Xiang-Gao WangORCID; En-Wei LiangORCID

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

Pp. L14

A Shining Death of Unequal Supermassive Black Hole Binaries

Xian ChenORCID; D. N. C. LinORCID; Xiaojia Zhang

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

Pp. L15