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
Spiral-wave Wind for the Blue Kilonova
Vsevolod Nedora
; Sebastiano Bernuzzi; David Radice; Albino Perego; Andrea Endrizzi; Néstor Ortiz
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L30
Evolving LMXBs: CARB Magnetic Braking
Kenny X. Van; Natalia Ivanova
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L31
Bright Gamma-Ray Flares Observed in GRB 131108A
M. Ajello; M. Arimoto; K. Asano; M. Axelsson; L. Baldini; G. Barbiellini; D. Bastieri; R. Bellazzini; A. Berretta; E. Bissaldi; R. D. Blandford; R. Bonino; E. Bottacini; J. Bregeon; P. Bruel; R. Buehler; S. Buson; R. A. Cameron; R. Caputo; P. A. Caraveo; E. Cavazzuti; S. Chen; G. Chiaro; S. Ciprini; D. Costantin; S. Cutini; F. D’Ammando; P. de la Torre Luque; F. de Palma; N. Di Lalla; L. Di Venere; F. Fana Dirirsa; S. J. Fegan; A. Franckowiak; Y. Fukazawa; P. Fusco; F. Gargano; D. Gasparrini; N. Giglietto; F. Giordano; M. Giroletti; D. Green; I. A. Grenier; M.-H. Grondin; S. Guiriec; E. Hays; D. Horan; G. Jóhannesson; D. Kocevski; M. Kovac’evic’; M. Kuss; S. Larsson; L. Latronico; J. Li; I. Liodakis; F. Longo; F. Loparco; M. N. Lovellette; P. Lubrano; S. Maldera; A. Manfreda; G. Martí-Devesa; M. N. Mazziotta; J. E. McEnery; I. Mereu; P. F. Michelson; T. Mizuno; M. E. Monzani; E. Moretti; A. Morselli; I. V. Moskalenko; M. Negro; E. Nuss; M. Ohno; N. Omodei; M. Orienti; E. Orlando; M. Palatiello; V. S. Paliya; D. Paneque; Z. Pei; M. Persic; M. Pesce-Rollins; V. Petrosian; F. Piron; H. Poon; T. A. Porter; G. Principe; J. L. Racusin; S. Rainò; R. Rando; B. Rani; M. Razzano; A. Reimer; O. Reimer; D. Serini; C. Sgrò; E. J. Siskind; G. Spandre; P. Spinelli; H. Tajima; K. Takagi; D. Tak; D. F. Torres; J. Valverde; K. Wood; R. Yamazaki; M. Yassine; S. Zhu; Z. Lucas Uhm; Bing Zhang
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L33
The Formation of CME from Coupling Fan-spine Magnetic System: A Difficult Journey
Haidong Li; Jiayan Yang; Junchao Hong; Hechao Chen
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L34
ALMA C ii 158 μm Imaging of an H i-selected Major Merger at z ∼ 4
J. Xavier Prochaska; Marcel Neeleman; Nissim Kanekar; Marc Rafelski
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L35
Laboratory Experiments on the Motion of Dense Dust Clouds in Protoplanetary Disks
Niclas Schneider; Gerhard Wurm
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L36
MESSENGER Observations of Giant Plasmoids in Mercury’s Magnetotail
J. Zhong; Q. G. Zong; Y. Wei; J. A. Slavin; X. Cao; Z. Y. Pu; X. G. Wang; S. Y. Fu; J. M. Raines; W. X. Wan
<jats:title>Abstract</jats:title> <jats:p>Small-scale flux ropes, with estimated diameters of ∼500 km and that pass over the <jats:italic>MESSENGER</jats:italic> spacecraft on timescales of seconds or less, are a common feature in Mercury’s magnetosphere. These magnetic structures, sometimes referred to as plasmoids, are believed to form as a result of rapid transient reconnection in the cross-tail current sheet at Mercury and the other planets. Here we report the occurrence of unusually large plasmoids in Mercury’s magnetotail observed, by the <jats:italic>MESSENGER</jats:italic> spacecraft. These plasmoids are remarkable for several reasons. Their spatial scales in the north–south direction exceed Mercury’s radius of 2440 km, and their time durations are comparable to or longer than the average Dungey cycle time of ∼200 s. They also have a more loop-like magnetic structure than the more common helical-like flux rope topology. These new <jats:italic>MESSENGER</jats:italic> observations suggest that Mercury’s magnetosphere can dissipate large quantities of magnetic flux and energy not only through the formation of a large number of small flux ropes, but also occasionally by the formation and release of a single giant plasmoid.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L32
Frequency of Coronal Mass Ejection Impacts with Early Terrestrial Planets and Exoplanets around Active Solar-like Stars
Christina Kay; Vladimir S. Airapetian; Theresa Lüftinger; Oleg Kochukhov
<jats:title>Abstract</jats:title> <jats:p>Energetic flares and associated coronal mass ejections (CMEs) from young magnetically active solar-like stars can play a critical role in setting conditions for atmospheric escape as well as penetration of accelerated particles into their atmospheres that promotes formation of biologically relevant molecules. We have used the observationally reconstructed magnetic field of the 0.7 Gyr young Sun’s twin, <jats:italic>k</jats:italic> <jats:sup>1</jats:sup> <jats:italic>Ceti</jats:italic>, to study the effects of CME deflections in the magnetic corona of the young Sun and their effects on the impact frequency on the early Venus, Earth, and Mars. We find that the coronal magnetic field deflects the CMEs toward the astrospheric current sheet. This effect suggests that CMEs tend to propagate within a small cone about the ecliptic plane increasing the impact frequency of CMEs with planetary magnetospheres near this plane to ∼30% or by a factor of 6 as compared to previous estimate by Airapetian et al. Our model has important implications for the rise of prebiotic chemistry on early terrestrial planets as well as terrestrial-type exoplanets around young G-K dwarfs.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L37
Asteroseismic Constraints on the Cosmic-time Variation of the Gravitational Constant from an Ancient Main-sequence Star
Earl Patrick Bellinger; Jørgen Christensen-Dalsgaard
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L1
Heavy Ion Acceleration by Super-Alfvénic Waves
S. Matsukiyo; T. Akamizu; T. Hada
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L2