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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

Compact Elliptical Galaxies Hosting Active Galactic Nuclei in Isolated Environments

Soo-Chang ReyORCID; Kyuseok OhORCID; Suk KimORCID

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

Pp. L9

Dark Matter Deficient Galaxies and Their Member Star Clusters Form Simultaneously during High-velocity Galaxy Collisions in 1.25 pc Resolution Simulations

Joohyun LeeORCID; Eun-jin ShinORCID; Ji-hoon KimORCID

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

Pp. L15

Modeling the Observed Distortion of Multiple (Ghost) CME Fronts in STEREO Heliospheric Imagers

Yutian ChiORCID; Christopher ScottORCID; Chenglong ShenORCID; Luke BarnardORCID; Mathew OwensORCID; Mengjiao XuORCID; Jie ZhangORCID; Shannon Jones; Zhihui ZhongORCID; Bingkun YuORCID; Matthew Lang; Yuming WangORCID; Mike LockwoodORCID

<jats:title>Abstract</jats:title> <jats:p>In this work we have, for the first time, applied the interpretation of multiple “ghost-fronts” to two synthetic coronal mass ejections (CMEs) propagating within a structured solar wind using the Heliospheric Upwind eXtrapolation time (HUXt) solar wind model. The two CMEs occurred on 2012 June 13–14 showing multiple fronts in images from Solar Terrestrial Relations Observatory Heliospheric Imagers (HIs). The HUXt model is used to simulate the evolution of these CMEs across the inner heliosphere as they interacted with structured ambient solar wind. The simulations reveal that the evolution of CME shape is consistent with observations across a wide range of solar latitudes and that the manifestation of multiple “ghost-fronts” within HIs’ field of view is consistent with the positions of the nose and flank of the same CME structure. This provides further confirmation that the angular separation of these features provides information on the longitudinal extent of a CME. For one of the CMEs considered in this study, both simulations and observations show that a concave shape develops within the outer CME front. We conclude that this distortion results from a latitudinal structure in the ambient solar wind speed. The work emphasizes that the shape of the CME cannot be assumed to remain a coherent geometrical shape during its propagation in the heliosphere. Our analysis demonstrates that the presence of “ghost” CME fronts can be used to infer the distortion of CMEs by ambient solar wind structure as a function of both latitude and longitude. This information has the potential to improve the forecasting of space weather events at Earth.</jats:p>

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

Pp. L16

An Ancient Massive Quiescent Galaxy Found in a Gas-rich z ∼ 3 Group

Boris S. KalitaORCID; Emanuele DaddiORCID; Chiara D’EugenioORCID; Francesco ValentinoORCID; R. Michael RichORCID; Carlos Gómez-GuijarroORCID; Rosemary T. CooganORCID; Ivan DelvecchioORCID; David ElbazORCID; James D. NeillORCID; Annagrazia PuglisiORCID; Veronica StrazzulloORCID

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

Pp. L17

A Corotating Group of Dwarf Galaxies around NGC 2750 as a Centaurus A Analog

Sanjaya PaudelORCID; Suk-Jin YoonORCID; Rory SmithORCID

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

Pp. L18

On the Evidence for a Common-spectrum Process in the Search for the Nanohertz Gravitational-wave Background with the Parkes Pulsar Timing Array

Boris GoncharovORCID; R. M. ShannonORCID; D. J. ReardonORCID; G. Hobbs; A. ZicORCID; M. BailesORCID; M. Curyło; S. DaiORCID; M. KerrORCID; M. E. LowerORCID; R. N. ManchesterORCID; R. MandowORCID; H. MiddletonORCID; M. T. Miles; A. ParthasarathyORCID; E. ThraneORCID; N. ThyagarajanORCID; X. Xue; X.-J. ZhuORCID; A. D. CameronORCID; Y. FengORCID; R. LuoORCID; C. J. RussellORCID; J. Sarkissian; R. SpiewakORCID; S. WangORCID; J. B. WangORCID; L. ZhangORCID; S. Zhang

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

Pp. L19

Magnetic Field Draping of the Heliopause and Its Consequences for Radio Emission in the Very Local Interstellar Medium

N. V. PogorelovORCID; F. FraternaleORCID; T. K. KimORCID; L. F. BurlagaORCID; D. A. GurnettORCID

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

Pp. L20

Solar-cycle Variations of South Atlantic Anomaly Proton Intensities Measured with the PAMELA Mission

A. BrunoORCID; M. MartucciORCID; F. S. CafagnaORCID; R. SparvoliORCID; O. AdrianiORCID; G. C. Barbarino; G. A. Bazilevskaya; R. Bellotti; M. BoezioORCID; E. A. Bogomolov; M. Bongi; V. Bonvicini; D. CampanaORCID; P. Carlson; M. CasolinoORCID; G. Castellini; C. De Santis; A. M. Galper; S. V. Koldashov; S. Koldobskiy; A. N. Kvashnin; A. Lenni; A. A. Leonov; V. V. Malakhov; L. Marcelli; N. Marcelli; A. G. Mayorov; W. MennORCID; M. Mergè; E. MocchiuttiORCID; A. Monaco; N. MoriORCID; V. V. MikhailovORCID; R. MuniniORCID; G. OsteriaORCID; B. Panico; P. Papini; M. PearceORCID; P. PicozzaORCID; M. RicciORCID; S. B. RicciariniORCID; M. Simon; A. Sotgiu; P. Spillantini; Y. I. Stozhkov; A. Vacchi; E. Vannuccini; G. I. Vasilyev; S. A. VoronovORCID; Y. T. Yurkin; G. Zampa; N. Zampa; T. R. Zharaspayev

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

Pp. L21

Bayesian Inference of Strange Star Equation of State Using the GW170817 and GW190425 Data

Zhiqiang MiaoORCID; Jin-Liang JiangORCID; Ang LiORCID; Lie-Wen ChenORCID

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

Pp. L22

Second Harmonic Electromagnetic Emissions by an Electron Beam in Solar Wind Plasmas with Density Fluctuations

C. KrafftORCID; P. Savoini

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

Pp. L23