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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

The Time Delay Distribution and Formation Metallicity of LIGO-Virgo’s Binary Black Holes

Maya FishbachORCID; Vicky KalogeraORCID

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

Pp. L30

Effect of H2S on the Near-infrared Spectrum of Irradiation Residue and Applications to the Kuiper Belt Object (486958) Arrokoth

Ahmed MahjoubORCID; Michael E. BrownORCID; Michael J. PostonORCID; Robert Hodyss; Bethany L. EhlmannORCID; Jordana Blacksberg; Mathieu ChoukrounORCID; John M. Eiler; Kevin P. HandORCID

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

Pp. L31

Targeted Modeling of GW150914's Binary Black Hole Source with Dart_board

Jeff J. AndrewsORCID; Julianne CroninORCID; Vicky KalogeraORCID; Christopher P. L. BerryORCID; Andreas ZezasORCID

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

Pp. L32

Modeling Interactions of Narrowband Large Amplitude Whistler-mode Waves with Electrons in the Solar Wind inside ∼0.3 au and at 1 au Using a Particle Tracing Code

Cynthia CattellORCID; Tien VoORCID

<jats:title>Abstract</jats:title> <jats:p>The discovery of large amplitude narrowband whistler-mode waves at frequencies of tenths of the electron cyclotron frequency in large numbers both inside ∼0.3 au and at ∼1 au provides an answer to longstanding questions about scattering and energization of solar wind electrons. The waves can have rapid nonlinear interactions with electrons over a broad energy range. Counter propagation between electrons and waves is not required for resonance with the obliquely propagating waves in contrast to the case for parallel propagation. Using a full 3D particle tracing code, we have examined interactions of electrons with energies from 0 eV to 2 keV with whistler-mode waves with amplitudes of 20 mV m<jats:sup>−1</jats:sup> and propagation angles from 0° to 180° to the background magnetic field. Interactions with wave packets and single waves are both modeled based on observations at ∼0.3 au and 1 au. A test particle simulation approach allows us to examine the particle motion in detail, which reveals kinetic effects of resonant interactions. The simulations demonstrate the key role played by these waves in rapid scattering and energization of electrons. Strong scattering and energization for some initial energy and pitch angle ranges occurs for both counter-propagating and obliquely propagating waves. Strong scattering of strahl electrons counteracts the pitch angle narrowing due to conservation of the first adiabatic invariant as electrons propagate from the Sun into regions of smaller magnetic field. Scattering also produces the hotter isotropic halo. The concomitant limiting of the electron heat flux is also relevant in other astrophysical settings.</jats:p>

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

Pp. L33

Do LIGO/Virgo Black Hole Mergers Produce AGN Flares? The Case of GW190521 and Prospects for Reaching a Confident Association

A. PalmeseORCID; M. FishbachORCID; C. J. BurkeORCID; J. AnnisORCID; X. LiuORCID

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

Pp. L34

Homologous Microflares with Mass Ejection and Plasma Heating on the Quiet Sun

C. L. JinORCID; G. P. ZhouORCID; J. X. WangORCID

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

Pp. L35

Proton Energization by Phase Steepening of Parallel-propagating Alfvénic Fluctuations

C. A. GonzálezORCID; A. TeneraniORCID; L. MatteiniORCID; P. HellingerORCID; M. VelliORCID

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

Pp. L36

The Challenge to MOND from Ultra-faint Dwarf Galaxies

Mohammadtaher SafarzadehORCID; Abraham LoebORCID

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

Pp. L37

Thermal Wave Instability as an Origin of Gap and Ring Structures in Protoplanetary Disks

Takahiro UedaORCID; Mario FlockORCID; Tilman BirnstielORCID

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

Pp. L38

The Double-bubble Coronal Mass Ejection of the 2020 December 14 Total Solar Eclipse

Benjamin BoeORCID; Bryan YamashiroORCID; Miloslav Druckmüller; Shadia HabbalORCID

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

Pp. L39