Catálogo de publicaciones - revistas
Título de Acceso Abierto
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
Cobertura temática
Tabla de contenidos
Compact Elliptical Galaxies Hosting Active Galactic Nuclei in Isolated Environments
Soo-Chang Rey; Kyuseok Oh; Suk Kim
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 Lee; Eun-jin Shin; Ji-hoon Kim
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 Chi; Christopher Scott; Chenglong Shen; Luke Barnard; Mathew Owens; Mengjiao Xu; Jie Zhang; Shannon Jones; Zhihui Zhong; Bingkun Yu; Matthew Lang; Yuming Wang; Mike Lockwood
<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. Kalita; Emanuele Daddi; Chiara D’Eugenio; Francesco Valentino; R. Michael Rich; Carlos Gómez-Guijarro; Rosemary T. Coogan; Ivan Delvecchio; David Elbaz; James D. Neill; Annagrazia Puglisi; Veronica Strazzullo
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 Paudel; Suk-Jin Yoon; Rory Smith
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 Goncharov; R. M. Shannon; D. J. Reardon; G. Hobbs; A. Zic; M. Bailes; M. Curyło; S. Dai; M. Kerr; M. E. Lower; R. N. Manchester; R. Mandow; H. Middleton; M. T. Miles; A. Parthasarathy; E. Thrane; N. Thyagarajan; X. Xue; X.-J. Zhu; A. D. Cameron; Y. Feng; R. Luo; C. J. Russell; J. Sarkissian; R. Spiewak; S. Wang; J. B. Wang; L. Zhang; 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. Pogorelov; F. Fraternale; T. K. Kim; L. F. Burlaga; D. A. Gurnett
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. Bruno; M. Martucci; F. S. Cafagna; R. Sparvoli; O. Adriani; G. C. Barbarino; G. A. Bazilevskaya; R. Bellotti; M. Boezio; E. A. Bogomolov; M. Bongi; V. Bonvicini; D. Campana; P. Carlson; M. Casolino; 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. Menn; M. Mergè; E. Mocchiutti; A. Monaco; N. Mori; V. V. Mikhailov; R. Munini; G. Osteria; B. Panico; P. Papini; M. Pearce; P. Picozza; M. Ricci; S. B. Ricciarini; M. Simon; A. Sotgiu; P. Spillantini; Y. I. Stozhkov; A. Vacchi; E. Vannuccini; G. I. Vasilyev; S. A. Voronov; 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 Miao; Jin-Liang Jiang; Ang Li; Lie-Wen Chen
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L22