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 Pulsating White Dwarf G117-B15A: Still the Most Stable Optical Clock Known
S. O. Kepler
; D. E. Winget; Zachary P. Vanderbosch; Barbara Garcia Castanheira; J. J. Hermes; Keaton J. Bell; Fergal Mullally; Alejandra D. Romero; M. H. Montgomery; Steven DeGennaro; Karen I. Winget; Dean Chandler; Elizabeth J. Jeffery; Jamile K. Fritzen; Kurtis A. Williams; Paul Chote; Staszek Zola
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 7
Lorentz Invariance Violation Limits from the Spectral-lag Transition of GRB 190114C
Shen-Shi Du; Lin Lan; Jun-Jie Wei; Zi-Min Zhou; He Gao; Lu-Yao Jiang; Bin-Bin Zhang; Zi-Ke Liu; Xue-Feng Wu; En-Wei Liang; Zong-Hong Zhu
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 8
Investigating the Mini and Giant Radio Flare Episodes of Cygnus X-3
Elise Egron; Alberto Pellizzoni; Simona Righini; Marcello Giroletti; Karri Koljonen; Katja Pottschmidt; Sergei Trushkin; Jessica Lobina; Maura Pilia; Joern Wilms; Stéphane Corbel; Victoria Grinberg; Sara Loru; Alessio Trois; Jérome Rodriguez; A. Lähteenmäki; M. Tornikoski; S. Enestam; E. Järvelä
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 10
A Variable Ionized Disk Wind in the Black Hole Candidate EXO 1846–031
Yanan Wang; Long Ji; Javier A. García; Thomas Dauser; Mariano Méndez; Junjie Mao; L. Tao; Diego Altamirano; Pierre Maggi; S. N. Zhang; M. Y. Ge; L. Zhang; J. L. Qu; S. Zhang; X. Ma; F. J. Lu; T. P. Li; Y. Huang; S. J. Zheng; Z. Chang; Y. L. Tuo; L. M. Song; Y. P. Xu; Y. Chen; C. Z. Liu; Q. C. Bu; C. Cai; X. L. Cao; L. Chen; T. X. Chen; Y. P. Chen; W. W. Cui; Y. Y. Du; G. H. Gao; Y. D. Gu; J. Guan; C. C. Guo; D. W. Han; J. Huo; S. M. Jia; W. C. Jiang; J. Jin; L. D. Kong; B. Li; C. K. Li; G. Li; W. Li; X. Li; X. B. Li; X. F. Li; Z. W. Li; X. H. Liang; J. Y. Liao; H. W. Liu; X. J. Liu; X. F. Lu; Q. Luo; T. Luo; B. Meng; Y. Nang; J. Y. Nie; G. Ou; N. Sai; R. C. Shang; X. Y. Song; L. Sun; Y. Tan; W. S. Wang; Y. D. Wang; Y. S. Wang; X. Y. Wen; B. B. Wu; B. Y. Wu; M. Wu; G. C. Xiao; S. Xiao; S. L. Xiong; S. Yang; Y. J. Yang; Q. B. Yi; Q. Q. Yin; Y. You; F. Zhang; H. M. Zhang; J. Zhang; W. C. Zhang; W. Zhang; Y. F. Zhang; H. S. Zhao; X. F. Zhao; D. K. Zhou
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 11
A Closer Look at Two of the Most Luminous Quasars in the Universe
Jan-Torge Schindler; Xiaohui Fan; Mladen Novak; Bram Venemans; Fabian Walter; Feige Wang; Jinyi Yang; Minghao Yue; Eduardo Bañados; Yun-Hsin Huang
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 12
Superorbital Modulation in the High-mass X-Ray Binary 4U 1538–52 and Possible Modulation in IGR J16393–4643
Robin H. D. Corbet; Joel B. Coley; Hans A. Krimm; Katja Pottschmidt; Paul Roche
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 13
A New Feedback Cycle in the Archetypal Cooling Flow Group NGC 5044
Gerrit Schellenberger; Laurence P. David; Jan Vrtilek; Ewan O’Sullivan; Simona Giacintucci; William Forman; Christine Jones; Tiziana Venturi
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 16
Excitation of Spin–Orbit Misalignments in Stellar Binaries with Circumbinary Disks: Application to DI Herculis
Kassandra R. Anderson; Dong Lai
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 17
Monte Carlo Applications for Partially Polarized Inverse External-Compton Scattering (MAPPIES). I. Description of the Code and First Results
Lenté Dreyer; Markus Böttcher
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 18
Plumelets: Dynamic Filamentary Structures in Solar Coronal Plumes
V. M. Uritsky; C. E. DeForest; J. T. Karpen; C. R. DeVore; P. Kumar; N. E. Raouafi; P. F. Wyper
<jats:title>Abstract</jats:title> <jats:p>Solar coronal plumes long seemed to possess a simple geometry supporting spatially coherent, stable outflow without significant fine structure. Recent high-resolution observations have challenged this picture by revealing numerous transient, small-scale, collimated outflows (“jetlets”) at the base of plumes. The dynamic filamentary structure of solar plumes above these outflows, and its relationship with the overall plume structure, have remained largely unexplored. We analyzed the statistics of continuously observed fine structure inside a single representative bright plume within a mid-latitude coronal hole during 2016 July 2–3. By applying advanced edge-enhancement and spatiotemporal analysis techniques to extended series of high-resolution images from the Solar Dynamics Observatory's Atmospheric Imaging Assembly, we determined that the plume was composed of numerous time-evolving filamentary substructures, referred to as “plumelets” in this paper, that accounted for most of the plume emission. The number of simultaneously identifiable plumelets was positively correlated with plume brightness, peaked in the fully formed plume, and remained saturated thereafter. The plumelets had transverse widths of 10 Mm and intermittently supported upwardly propagating periodic disturbances with phase speeds of 190–260 km s<jats:sup>−1</jats:sup> and longitudinal wavelengths of 55–65 Mm. The characteristic frequency (≈ 3.3 mHz) is commensurate with that of solar <jats:italic>p</jats:italic>-modes. Oscillations in neighboring plumelets are uncorrelated, indicating that the waves could be driven by <jats:italic>p</jats:italic>-mode flows at spatial scales smaller than the plumelet separation. Multiple independent sources of outflow within a single coronal plume should impart significant fine structure to the solar wind that may be detectable by Parker Solar Probe and Solar Orbiter.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 1