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
TOI-942b: A Prograde Neptune in a ∼ 60 Myr Old Multi-transiting System*
Christopher P. Wirth
; George Zhou; Samuel N. Quinn; Andrew W. Mann; Luke G. Bouma; David W. Latham; Johanna K. Teske; Sharon X. Wang; Stephen A. Shectman; R. P. Butler; Jeffrey D. Crane
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L34
PAH Spectroscopy from 1 to 5 μm
L. J. Allamandola; C. Boersma; T. J. Lee; J. D. Bregman; P. Temi
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L35
The Detection of Ionized Carbon Emission at z ∼ 8*
Michael W. Topping; Alice E. Shapley; Daniel P. Stark; Ryan Endsley; Brant Robertson; Jenny E. Greene; Steven R. Furlanetto; Mengtao Tang
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L36
A Short Mean Free Path at z = 6 Favors Late and Rapid Reionization by Faint Galaxies
Christopher Cain; Anson D’Aloisio; Nakul Gangolli; George D. Becker
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L37
Luminosity Dependence of the Cyclotron Line Energy in 1A 0535+262 Observed by Insight-HXMT during the 2020 Giant Outburst
L. D. Kong; S. Zhang; L. Ji; P. Reig; V. Doroshenko; A. Santangelo; R. Staubert; S. N. Zhang; R. Soria; Z. Chang; Y. P. Chen; P. J. Wang; L. Tao; J. L. Qu
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L38
Cosmic-Ray Acceleration from Turbulence in Molecular Clouds
Brandt A. L. Gaches; Stefanie Walch; A. Lazarian
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L39
Erratum: Dust Polarization in Four Protoplanetary Disks at 3 mm: Further Evidence of Multiple Origins (2019, ApJL, 877, L2)
Rachel E. Harrison; Leslie W. Looney; Ian W. Stephens; Zhi-Yun Li; Haifeng Yang; Akimasa Kataoka; Robert J. Harris; Woojin Kwon; Takayuki Muto; Munetake Momose
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L40
The Nature and Composition of Jupiter’s Building Blocks Derived from the Water Abundance Measurements by the Juno Spacecraft
Olivier Mousis; Jonathan I. Lunine; Artyom Aguichine
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L23
Formation of Multiple Populations of M5 (NGC 5904)
Jae-Woo Lee
<jats:title>Abstract</jats:title> <jats:p>With our new Ca-CN-CH-NH photometry, we revisit the globular cluster (GC) M5. We find that M5 is a mono-metallic GC with a small metallicity dispersion. Our carbon abundances show that the <jats:italic>σ</jats:italic>[C/Fe] of the M5 CN-s population, with depleted carbon and enhanced nitrogen abundances, is significantly large for a single stellar population. Our new analysis reveals that the M5 CN-s population is well described by the two stellar populations: the CN-s<jats:sub>I</jats:sub>, being the major CN-s component, with the intermediate carbon and nitrogen abundance and the CN-s<jats:sub>E</jats:sub> with the most carbon-poor and nitrogen-rich abundance. We find that the CN-s<jats:sub>E</jats:sub> is significantly more centrally concentrated than the others, while CN-w and CN-s<jats:sub>I</jats:sub> have similar cumulative radial distributions. The red giant branch bump <jats:italic>V</jats:italic> magnitude, the helium abundance barometer in mono-metallic populations, of individual populations appears to be correlated with their mean carbon abundance, indicating that carbon abundances are anticorrelated with helium abundances. We propose that the CN-s<jats:sub>E</jats:sub> formed out of gas that experienced proton-capture processes at high temperatures in the innermost region of the proto-GC of M5 that resided in a dense ambient density environment. Shortly after, the CN-s<jats:sub>I</jats:sub> formed out of gas diluted from the pristine gas in the more spatially extended region, consistent with the current development of numerical simulations by others.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L24
On the Detection of Exomoons Transiting Isolated Planetary-mass Objects
Mary Anne Limbach; Johanna M. Vos; Joshua N. Winn; René Heller; Jeffrey C. Mason; Adam C. Schneider; Fei Dai
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L25