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
CO Detected in CI Tau b: Hot Start Implied by Planet Mass and M K
Laura Flagg
; Christopher M. Johns-Krull; Larissa Nofi; Joe Llama; L. Prato; Kendall Sullivan; D. T. Jaffe; Gregory Mace
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L37
Double Detonations with Thin, Modestly Enriched Helium Layers can Make Normal Type Ia Supernovae
Dean M. Townsley; Broxton J. Miles; Ken J. Shen; Daniel Kasen
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L38
Erratum: “A Luminous Red Nova in M31 and its Progenitor System” (2015, ApJ, 805, L18)
S. C. Williams; M. J. Darnley; M. F. Bode; I. A. Steele
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L39
Circumgalactic Pressure Profiles Indicate Precipitation-limited Atmospheres for M * ∼ 109–1011.5 M ⊙
G. Mark Voit; Megan Donahue; Fakhri Zahedy; Hsiao-Wen Chen; Jessica Werk; Greg L. Bryan; Brian W. O’Shea
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L1
PDS 70: A Transition Disk Sculpted by a Single Planet
Dhruv Muley; Jeffrey Fung; Nienke van der Marel
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L2
The Mass Function of Supermassive Black Holes in the Direct-collapse Scenario
Shantanu Basu; Arpan Das
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L3
Hard-state Accretion Disk Winds from Black Holes: The Revealing Case of MAXI J1820+070
T. Muñoz-Darias; F. Jiménez-Ibarra; G. Panizo-Espinar; J. Casares; D. Mata Sánchez; G. Ponti; R. P. Fender; D. A. H. Buckley; P. Garnavich; M. A. P. Torres; M. Armas Padilla; P. A. Charles; J. M. Corral-Santana; J. J. E. Kajava; E. J. Kotze; C. Littlefield; J. Sánchez-Sierras; D. Steeghs; J. Thomas
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L4
The Supersoft X-Ray Transient ASASSN-16oh as a Thermonuclear Runaway without Mass Ejection
Yael Hillman; Marina Orio; Dina Prialnik; Michael Shara; Pavol Bezák; Andrej Dobrotka
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L5
Double-peaked [O i] Profile: A Likely Signature of the Gaseous Ring around KH 15D
Min Fang; Ilaria Pascucci; Jinyoung Serena Kim; Suzan Edwards
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L10
Helium Variation across Two Solar Cycles Reveals a Speed-dependent Phase Lag
B. L. Alterman; Justin C. Kasper
<jats:title>Abstract</jats:title> <jats:p>We study the relationship between the solar wind helium-to-hydrogen abundance ratio (<jats:italic>A</jats:italic> <jats:sub>He</jats:sub>), solar wind speed (<jats:italic>v</jats:italic> <jats:sub>sw</jats:sub>), and sunspot number (SSN) over solar cycles 23 and 24. This is the first full 22 year Hale cycle measured with the <jats:italic>Wind</jats:italic> spacecraft covering a full cycle of the solar dynamo with two polarity reversals. While previous studies have established a strong correlation between <jats:italic>A</jats:italic> <jats:sub>He</jats:sub> and SSN, we show that the phase delay between <jats:italic>A</jats:italic> <jats:sub>He</jats:sub> and SSN is a monotonic increasing function of <jats:italic>v</jats:italic> <jats:sub>sw</jats:sub>. Correcting for this lag, <jats:italic>A</jats:italic> <jats:sub>He</jats:sub> returns to the same value at a given SSN over all rising and falling phases and across solar wind speeds. We infer that this speed-dependent lag is a consequence of the mechanism that depletes slow wind <jats:italic>A</jats:italic> <jats:sub>He</jats:sub> from its fast wind value during solar wind formation.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L6