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
In-situ Switchback Formation in the Expanding Solar Wind
J. Squire
; B. D. G. Chandran; R. Meyrand
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L2
Detecting Interstellar Objects through Stellar Occultations
Amir Siraj; Abraham Loeb
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L3
De-noising SDO/HMI Solar Magnetograms by Image Translation Method Based on Deep Learning
Eunsu Park; Yong-Jae Moon; Daye Lim; Harim Lee
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L4
Nine New Repeating Fast Radio Burst Sources from CHIME/FRB
E. Fonseca; B. C. Andersen; M. Bhardwaj; P. Chawla; D. C. Good; A. Josephy; V. M. Kaspi; K. W. Masui; R. Mckinven; D. Michilli; Z. Pleunis; K. Shin; S. P. Tendulkar; K. M. Bandura; P. J. Boyle; C. Brar; T. Cassanelli; D. Cubranic; M. Dobbs; F. Q. Dong; B. M. Gaensler; G. Hinshaw; T. L. Landecker; C. Leung; D. Z. Li; H.-H. Lin; J. Mena-Parra; M. Merryfield; A. Naidu; C. Ng; C. Patel; U. Pen; M. Rafiei-Ravandi; M. Rahman; S. M. Ransom; P. Scholz; K. M. Smith; I. H. Stairs; K. Vanderlinde; P. Yadav; A. V. Zwaniga
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L6
Onset of Cosmic Reionization: Evidence of an Ionized Bubble Merely 680 Myr after the Big Bang
V. Tilvi; S. Malhotra; J. E. Rhoads; A. Coughlin; Z. Zheng; S. L. Finkelstein; S. Veilleux; B. Mobasher; J. Wang; R. Probst; R. Swaters; P. Hibon; B. Joshi; J. Zabl; T. Jiang; J. Pharo; H. Yang
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L10
Laboratory Observations of Ultra-low-frequency Analog Waves Driven by the Right-hand Resonant Ion Beam Instability
Peter V. Heuer; Martin. S. Weidl; Robert S. Dorst; Derek B. Schaeffer; Shreekrishna K. P. Tripathi; Stephen Vincena; Carmen G. Constantin; Christoph Niemann; Lynn B. Wilson III; Dan Winske
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L11
The Formation Height of Millimeter-wavelength Emission in the Solar Chromosphere
Juan Martínez-Sykora; Bart De Pontieu; Jaime de la Cruz Rodriguez; Georgios Chintzoglou
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L8
Newly Discovered Source of Turbulence and Heating in the Solar Chromosphere
Meers Oppenheim; Yakov Dimant; William Longley; Alex C. Fletcher
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L9
The Mysterious Location of Maryland on 2014 MU69 and the Reconfiguration of Its Bilobate Shape
Masatoshi Hirabayashi; Alexander J. Trowbridge; Dennis Bodewits
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L12
Two-component Jets of GRB 160623A as Shocked Jet Cocoon Afterglow
Wei Ju Chen; Yuji Urata; Kuiyun Huang; Satoko Takahashi; Glen Petitpas; Keiichi Asada
<jats:title>Abstract</jats:title> <jats:p>Two components of jets associated with the afterglow of the gamma-ray burst (GRB) 160623A were observed with multifrequency observations including long-term monitoring in a submillimeter range (230 GHz) using the Submillimeter Array. The observed light curves with temporal breaks suggest on the basis of the standard forward-shock synchrotron-radiation model that the X-ray radiation is narrowly collimated with an opening angle <jats:inline-formula> <jats:tex-math> <?CDATA ${\theta }_{n,j}\lt \sim 6^\circ $?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjlab76d4ieqn1.gif" xlink:type="simple" /> </jats:inline-formula>, whereas the radio radiation originated from wider jets (∼27°). The temporal and spectral evolutions of the radio afterglow agree with those expected from a synchrotron-radiation modeling with typical physical parameters, except for the fact that the observed wide jet opening angle for the radio emission is significantly larger than the theoretical maximum opening angle. By contrast, the opening angle of the X-ray afterglow is consistent with the typical value of GRB jets. Since the theory of the relativistic cocoon afterglow emission is similar to that of a regular afterglow with an opening angle of ∼30°, the observed radio emission can be interpreted as the shocked jet cocoon emission. This result therefore indicates that the two components of the jets observed in the GRB 160623A afterglow are caused by the jet and the shocked jet cocoon afterglows.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L15