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
NICER Observes a Secondary Peak in the Decay of a Thermonuclear Burst from 4U 1608–52
Gaurava K. Jaisawal
; Jérôme Chenevez; Peter Bult; Jean J. M. in’t Zand; Duncan K. Galloway; Tod E. Strohmayer; Tolga Güver; Phillip Adkins; Diego Altamirano; Zaven Arzoumanian; Deepto Chakrabarty; Jonathan Coopersmith; Keith C. Gendreau; Sebastien Guillot; Laurens Keek; Renee M. Ludlam; Christian Malacaria
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 61
Origin and Evolution of Distinct Molybdenum Isotopic Variabilities within Carbonaceous and Noncarbonaceous Reservoirs
Tetsuya Yokoyama; Yuichiro Nagai; Ryota Fukai; Takafumi Hirata
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 62
Machine-learning Classifiers for Intermediate Redshift Emission-line Galaxies
Kai Zhang; David J. Schlegel; Brett H. Andrews; Johan Comparat; Christoph Schäfer; Jose Antonio Vazquez Mata; Jean-Paul Kneib; Renbin Yan
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 63
Spectral Properties of Populations Behind the Coherence in Spitzer Near-infrared and Chandra X-Ray Backgrounds
Yanxia Li; Nico Cappelluti; Günther Hasinger; Richard G. Arendt; Alexander Kashlinsky; Fabio Pacucci
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 64
Signatures of Magnetic Activity: On the Relation between Stellar Properties and p-mode Frequency Variations
A. R. G. Santos; T. L. Campante; W. J. Chaplin; M. S. Cunha; J. L. van Saders; C. Karoff; T. S. Metcalfe; S. Mathur; R. A. García; M. N. Lund; R. Kiefer; V. Silva Aguirre; G. R. Davies; R. Howe; Y. Elsworth
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 65
Inverse Compton Cascades in Pair-producing Gaps: Effects of Triplet Pair Production
Maria Petropoulou; Yajie Yuan; Alexander Y. Chen; Apostolos Mastichiadis
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 66
Solar Angular Momentum Loss over the Past Several Millennia
Adam J. Finley; Siddhant Deshmukh; Sean P. Matt; Mathew Owens; Chi-Ju Wu
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 67
Sculpting Eccentric Debris Disks with Eccentric Gas Rings
Jonathan W. Lin; Eugene Chiang
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 68
Numerical Simulation of Magnetic Reconnection around a Black Hole
Mika Inda-Koide; Shinji Koide; Ryogo Morino
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 69
New Spatially Resolved Imaging of the SR 21 Transition Disk and Constraints on the Small-grain Disk Geometry
S. Sallum; A. J. Skemer; J. A. Eisner; N. van der Marel; P. D. Sheehan; L. M. Close; M. J. Ireland; J. M. Males; K. M. Morzinski; V. P. Bailey; R. Briguglio; A. Puglisi
<jats:title>Abstract</jats:title> <jats:p>We present new 0.6–4 <jats:italic>μ</jats:italic>m imaging of the SR 21 transition disk from Keck/NIRC2 and Magellan/MagAO. The protoplanetary disk around SR 21 has a large (∼30–40 au) clearing first inferred from its spectral energy distribution and later detected in submillimeter imaging. Both the gas and small dust grains are known to have a different morphology, with an inner truncation in CO at ∼7 au, and micron-sized dust detected within the millimeter clearing. Previous near-infrared imaging could not distinguish between an inner dust disk with a truncation at ∼7 au or one that extended to the sublimation radius. The imaging data presented here require an inner dust disk radius of a few au, and complex structure such as a warp or spiral. We present a parametric warped disk model that can reproduce the observations. Reconciling the images with the spectral energy distribution gathered from the literature suggests grain growth to ≳2–5 <jats:italic>μ</jats:italic>m within the submillimeter clearing. The complex disk structure and possible grain growth can be connected to dynamical shaping by a giant-planet-mass companion, a scenario supported by previous observational and theoretical studies.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 100