Catálogo de publicaciones - revistas
Título de Acceso Abierto
The Astrophysical Journal (ApJ)
Resumen/Descripción – provisto por la editorial en inglés
The Astrophysical Journal is an open access journal devoted to recent developments, discoveries, and theories in astronomy and astrophysics. Publications in ApJ constitute significant new research that is directly relevant to astrophysical applications, whether based on observational results or on theoretical insights or modeling.Palabras clave – provistas por la editorial
astronomy; astrophysics
Disponibilidad
| Institución detectada | Período | Navegá | Descargá | Solicitá |
|---|---|---|---|---|
| No detectada | desde jul. 1995 / hasta dic. 2023 | IOPScience |
Información
Tipo de recurso:
revistas
ISSN impreso
0004-637X
ISSN electrónico
1538-4357
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
Sulfur-bearing Molecules in Orion KL
Gan Luo
; Siyi Feng; Di Li; Sheng-Li Qin; Yaping Peng; Ningyu Tang; Zhiyuan Ren; Hui Shi
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 82
Manifestations of Three-dimensional Magnetic Reconnection in an Eruption of a Quiescent Filament: Filament Strands Turning to Flare Loops
Juraj Lörinčík; Jaroslav Dudík; Guillaume Aulanier
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 83
The Central Star of NGC 2346 as a Clue to Binary Evolution through the Common Envelope Phase
M. A. Gómez-Muñoz; A. Manchado; L. Bianchi; M. Manteiga; R. Vázquez
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 84
DASH: Deep Learning for the Automated Spectral Classification of Supernovae and Their Hosts
Daniel Muthukrishna; David Parkinson; Brad E. Tucker
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 85
Hβ and Hγ Absorption-line Profile Inconsistencies in Laboratory Experiments Performed at White Dwarf Photosphere Conditions
M.-A. Schaeuble; T. Nagayama; J. E. Bailey; T. A. Gomez; M. H. Montgomery; D. E. Winget
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 86
The Imprint of Spiral Arms on the Galactic Rotation Curve
Stacy S. McGaugh
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 87
Dwarf Galaxy Discoveries from the KMTNet Supernova Program. II. The NGC 3585 Group and Its Dynamical State
Hong Soo Park; Dae-Sik Moon; Dennis Zaritsky; Sang Chul Kim; Youngdae Lee; Sang-Mok Cha; Yongseok Lee
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 88
Finding the Critical Decay Index in Solar Prominence Eruptions
N. Vasantharaju; P. Vemareddy; B. Ravindra; V. H. Doddamani
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 89
Solar Fast-drifting Radio Bursts in an X1.3 Flare on 2014 April 25
Baolin Tan; Naihwa Chen; Ya-Hui Yang; Chengming Tan; Satoshi Masuda; Xingyao Chen; H. Misawa
<jats:title>Abstract</jats:title> <jats:p>One of the most important products of solar flares is nonthermal energetic particles, which may carry up to 50% of the energy released in the flaring processes. In radio observations, nonthermal particles generally manifest as spectral fine structures with fast frequency-drifting rates, named as solar fast-drifting radio bursts (FDRBs). This work demonstrated three types of FDRBs, including type III pair bursts, narrowband stochastic spike bursts following the type III bursts, and spike-like bursts superimposed on a type II burst in an X1.3 flare on 2014 April 25. We find that although all of them have fast frequency-drifting rates, they are intrinsically different from each other in frequency bandwidth, drifting rate, and statistical distribution. We suggest that they are possibly generated from different accelerating mechanisms. The type III pair bursts may be triggered by high-energy electron beams accelerated by the flaring magnetic reconnection, spike bursts are produced by the energetic electrons accelerated by a termination shock wave triggered by the fast reconnecting plasma outflows impacting the flaring loop top, and spike-like bursts are possibly generated by nonthermal electrons accelerated by moving magnetic reconnection triggered by interaction between coronal mass ejection and the background magnetized plasma. These results may help us to understand the generation mechanism of nonthermal particles and energy release in solar flares.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 90
Including Dust Coagulation in Hydrodynamic Models of Protoplanetary Disks: Dust Evolution in the Vicinity of a Jupiter-mass Planet
Joanna Dra̧żkowska; Shengtai Li; Til Birnstiel; Sebastian M. Stammler; Hui Li
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 91