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
The Discovery of a Remnant Radio Galaxy in A2065 Using GMRT
Dharam V. Lal
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 126
Radio Emission by Soliton Formation in Relativistically Hot Streaming Pulsar Pair Plasmas
Jan Benáček; Patricio A. Muñoz; Alina C. Manthei; Jörg Büchner
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 127
Monte Carlo Investigation of the Ratios of Short-lived Radioactive Isotopes in the Interstellar Medium
Andrés Yagüe López; Benoit Côté; Maria Lugaro
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 128
Taking a Long Look: A Two-decade Reverberation Mapping Study of High-luminosity Quasars
Shai Kaspi; W. N. Brandt; Dan Maoz; Hagai Netzer; Donald P. Schneider; Ohad Shemmer; C. J. Grier
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 129
The Sandwich Mode for Vertical Shear Instability in Protoplanetary Disks
Thomas Pfeil; Hubert Klahr
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 130
The Architecture of the V892 Tau System: The Binary and Its Circumbinary Disk
Feng Long; Sean M. Andrews; Justin Vega; David J. Wilner; Claire J. Chandler; Enrico Ragusa; Richard Teague; Laura M. Pérez; Nuria Calvet; John M. Carpenter; Thomas Henning; Woojin Kwon; Hendrik Linz; Luca Ricci
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 131
Early Mass-varying Neutrino Dark Energy: Nugget Formation and Hubble Anomaly
Antareep Gogoi; Ravi Kumar Sharma; Prolay Chanda; Subinoy Das
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 132
Long-term Statistics of Pulsar Glitches Due to History-dependent Avalanches
Julian B. Carlin; Andrew Melatos
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 1
Do the Periodic Activities of Repeating Fast Radio Bursts Represent the Spins of Neutron Stars?
Kun Xu; Qiao-Chu Li; Yuan-Pei Yang; Xiang-Dong Li; Zi-Gao Dai; Jifeng Liu
<jats:title>Abstract</jats:title> <jats:p>Fast radio bursts (FRBs) are mysterious radio transients with millisecond durations. Recently, ∼16 days of periodic activity and ∼159 days of possible periodicity were detected to arise from FRB 180916.J0158+65 and FRB 121102, respectively, and the spin period of a slow-rotation magnetar was further considered to be one of the possible explanations of the periodic activities of repeating FRBs. For isolated neutron stars, the spin evolution suggests that it has difficulty reaching several hours. In this work, we mainly focus on the possible maximum spin period of isolated NSs/magnetars dominated by an interaction between a star’s magnetic field and the disk. We find that the disk wind plays an important role in spin evolution, whose influence varies the power-law index in the evolution equation of mass flow rate. For a magnetar without disk wind, the longest spin period is tens of hours. When the disk wind with a classical parameter is involved, the maximum spin period can reach hundreds of hours. But for an extremely large index of mass flow rate due to disk wind or other angular momentum extraction processes, a spin period of ∼(16–160) days is still possible.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 2
Excitation of Polycyclic Aromatic Hydrocarbon Emission: Dependence on Size Distribution, Ionization, and Starlight Spectrum and Intensity
B. T. Draine; Aigen Li; Brandon S. Hensley; L. K. Hunt; K. Sandstrom; J.-D. T. Smith
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 3