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
Asymmetry in the Length Scales of the Solar Supergranulation Network
K. P. Raju
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L35
Observations of a Radial Density Gradient in the Very Local Interstellar Medium by Voyager 2
W. S. Kurth; D. A. Gurnett
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L1
A Radio Pinwheel Emanating from WR 147
Luis F. Rodríguez; Jane Arthur; Gabriela Montes; Carlos Carrasco-González; Jesús A. Toalá
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L3
Different Fates of Young Star Clusters after Gas Expulsion
Xiaoying Pang; Yuqian Li; Shih-Yun Tang; Mario Pasquato; M. B. N. Kouwenhoven
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L4
Shock–Cloud Interaction in the Southwestern Rim of RX J1713.7–3946 Evidenced by Chandra X-Ray Observations
Takaaki Tanaka; Hiroyuki Uchida; Hidetoshi Sano; Takeshi Go Tsuru
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L5
Discovery of State Transition Behaviors in PSR J1124–5916
M. Y. Ge; J. P. Yuan; F. J. Lu; H. Tong; S. Q. Zhou; L. L. Yan; L. J. Wang; Y. L. Tuo; X. F. Li; L. M. Song
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L7
Detectability of Ultra-compact X-Ray Binaries as LISA Sources
Wen-Cong Chen; Dong-Dong Liu; Bo Wang
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L8
Early Science from GOTHAM: Project Overview, Methods, and the Detection of Interstellar Propargyl Cyanide (HCCCH2CN) in TMC-1
Brett A. McGuire; Andrew M. Burkhardt; Ryan A. Loomis; Christopher N. Shingledecker; Kin Long Kelvin Lee; Steven B. Charnley; Martin A. Cordiner; Eric Herbst; Sergei Kalenskii; Emmanuel Momjian; Eric R. Willis; Ci Xue; Anthony J. Remijan; Michael C. McCarthy
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L10
Solar Longitude Distribution of High-energy Proton Flares: Fluences and Spectra
E. W. Cliver; F. Mekhaldi; R. Muscheler
<jats:title>Abstract</jats:title> <jats:p>The distribution of the longitudes of solar flares associated with the high-energy proton events called ground level events (GLEs) can be approximated by a Gaussian with a peak at ∼W60, with a full range from ∼E90 to ∼W150. The longitudes of flares associated with the top third (24 of 72) of GLEs in terms of their >430 MeV fluences (<jats:italic>F</jats:italic> <jats:sub>430</jats:sub>) are primarily distributed over E20–W100 with a skew toward disk center. This 120° span in longitude is comparable to the latitudinal spans of powerful coronal mass ejections (CMEs) from limb flares. Only 5 of 24 strong GLEs are located within the W40–80 zone of good magnetic connection to Earth. GLEs with hard spectra, i.e., a spectral index SI<jats:sub>30/200</jats:sub>(= log(<jats:italic>F</jats:italic> <jats:sub>30</jats:sub>/<jats:italic>F</jats:italic> <jats:sub>200</jats:sub>)) < 1.5, also tend to avoid W40–80 source regions. Three-fourths of such events (16 of 21) arise in flares outside this range. The above tendencies favor a CME-driven shock source over a flare-resident acceleration process for high-energy solar protons. GLE spectra show a trend, with broad scatter, from hard spectra for events originating in eruptive flares beyond the west limb to soft spectra for GLEs with sources near central meridian. This behavior can be explained in terms of: (1) dominant near-Sun quasi-perpendicular shock acceleration of protons for far western (>W100) GLEs; (2) quasi-parallel shock acceleration for well-connected (W40–80) GLEs, and (3) proton acceleration/trapping at CME-driven bow shocks from central meridian (E20–W20) that strike the Earth.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L11
Short Gamma-Ray Bursts and the Decompression of Neutron Star Matter in Tidal Streams
C. J. Nixon; Eric R. Coughlin; J. E. Pringle
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L12