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
FAST Globular Cluster Pulsar Survey: Twenty-four Pulsars Discovered in 15 Globular Clusters
Zhichen Pan
; Lei Qian; Xiaoyun Ma; Kuo Liu; Lin Wang; Jintao Luo; Zhen Yan; Scott Ransom; Duncan Lorimer; Di Li; Peng Jiang
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L28
A Number of nearby Moving Groups May Be Fragments of Dissolving Open Clusters
Jonathan Gagné; Jacqueline K. Faherty; Leslie Moranta; Mark Popinchalk
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L29
Zero-metallicity Hypernova Uncovered by an Ultra-metal-poor Star in the Sculptor Dwarf Spheroidal Galaxy*
Ása Skúladóttir; Stefania Salvadori; Anish M. Amarsi; Eline Tolstoy; Michael J. Irwin; Vanessa Hill; Pascale Jablonka; Giuseppina Battaglia; Else Starkenburg; Davide Massari; Amina Helmi; Lorenzo Posti
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L30
Selection of Three (Extreme)Ultraviolet Channels for Solar Satellite Missions by Deep Learning
Daye Lim; Yong-Jae Moon; Eunsu Park; Jin-Yi Lee
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L31
Dependencies of Mantle Shock Heating in Pairwise Accretion
Travis S. J. Gabriel; Harrison Allen-Sutter
<jats:title>Abstract</jats:title> <jats:p>The final assembly of planets involves mutual collisions of large similar-sized protoplanets (“giant impacts”), setting the stage for modern geologic and atmospheric processes. However, thermodynamic consequences of impacts in diverse (exo)planetary systems/models are poorly understood. Impact velocity in “self-stirred” systems is proportional to the mass of the colliding bodies (<jats:italic>v</jats:italic> <jats:sub>imp</jats:sub> ∝ <jats:italic>M</jats:italic> <jats:sup>1/3</jats:sup>), providing a predictable transition to supersonic collisions in roughly Mars-sized bodies. In contrast, nearby larger planets, or migrating gas giants, stir impact velocities, producing supersonic collisions between smaller protoplanets and shifting outcomes to disruption and nonaccretion. Our particle hydrocode simulations suggest that thermodynamic processing can be enhanced in merging collisions more common to calmer dynamical systems due to post-impact processes that scale with the mass of the accreting remnant. Thus, impact heating can involve some contribution from energy scaling, a departure from pure velocity-scaling in cratering scenarios. Consequently, planetary thermal history depends <jats:italic>intimately</jats:italic> on the initial mass distribution assumptions and dynamical conditions of formation scenarios. In even the gentlest pairwise accretions, sufficiently large bodies feature debris fields dominated by melt and vapor. This likely plays a critical role in the observed diversity of exoplanet systems and certain debris disks. Furthermore, we suggest solar system formation models that involve self-stirred dynamics or only one to a few giant impacts between larger-than-Mars-sized bodies (e.g., “pebble accretion”) are more congruent with the “missing mantle problem” for the main belt, as we demonstrate debris would be predominantly vapor and thus less efficiently retained due to solar radiation pressure effects.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L32
Stars Lensed by the Supermassive Black Hole in the Center of the Milky Way: Predictions for ELT, TMT, GMT, and JWST
Michał J. Michałowski; Przemek Mróz
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L33
A Red Giant Branch Common-envelope Evolution Scenario for the Exoplanet WD 1856 b
Ariel Merlov; Ealeal Bear; Noam Soker
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L34
Evidence for Hierarchical Black Hole Mergers in the Second LIGO–Virgo Gravitational Wave Catalog
Chase Kimball; Colm Talbot; Christopher P L Berry; Michael Zevin; Eric Thrane; Vicky Kalogera; Riccardo Buscicchio; Matthew Carney; Thomas Dent; Hannah Middleton; Ethan Payne; John Veitch; Daniel Williams
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L35
A Preponderance of Perpendicular Planets
Simon H. Albrecht; Marcus L. Marcussen; Joshua N. Winn; Rebekah I. Dawson; Emil Knudstrup
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L1
A Circumplanetary Disk around PDS70c
Myriam Benisty; Jaehan Bae; Stefano Facchini; Miriam Keppler; Richard Teague; Andrea Isella; Nicolas T. Kurtovic; Laura M. Pérez; Anibal Sierra; Sean M. Andrews; John Carpenter; Ian Czekala; Carsten Dominik; Thomas Henning; Francois Menard; Paola Pinilla; Alice Zurlo
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L2