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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

https://creativecommons.org/licenses/by/4.0/

Cobertura temática

Tabla de contenidos

High-resolution Transmission Spectra of Earth Through Geological Time

Lisa KalteneggerORCID; Zifan LinORCID; Jack MaddenORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. L17

ALMA 50-parsec-resolution Imaging of Jet–ISM Interaction in the Lensed Quasar MG J0414+0534

Kaiki Taro InoueORCID; Satoki Matsushita; Kouichiro NakanishiORCID; Takeo MinezakiORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. L18

Planet-induced Vortices with Dust Coagulation in Protoplanetary Disks

Ya-Ping LiORCID; Hui LiORCID; Shengtai LiORCID; Tilman BirnstielORCID; Joanna Dra̧żkowskaORCID; Sebastian StammlerORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. L19

SDSS-IV MaNGA: Kinematic Asymmetry as an Indicator of Galaxy Interaction in Paired Galaxies

Shuai FengORCID; Shi-Yin ShenORCID; Fang-Ting Yuan; Rogemar A. RiffelORCID; Kaike PanORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. L20

A Well-aligned Orbit for the 45 Myr-old Transiting Neptune DS Tuc Ab

G. ZhouORCID; J. N. WinnORCID; E. R. NewtonORCID; S. N. QuinnORCID; J. E. RodriguezORCID; A. W. MannORCID; A. C. RizzutoORCID; A. M. VanderburgORCID; C. X. HuangORCID; D. W. LathamORCID; J. K. Teske; S. Wang; S. A. Shectman; R. P. ButlerORCID; J. D. CraneORCID; I. Thompson; T. J. Henry; L. A. Paredes; W. C. JaoORCID; H. S. James; R. Hinojosa

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. L21

Mass-shedding Activities of Asteroid (3200) Phaethon Enhanced by Its Rotation

Ryota NakanoORCID; Masatoshi HirabayashiORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. L22

CO, Water, and Tentative Methanol in η Carinae Approaching Periastron

Patrick W. MorrisORCID; Steven B. Charnley; Michael CorcoranORCID; Martin CordinerORCID; Augusto DamineliORCID; Jose H. Groh; Theodore R. GullORCID; Laurent LoinardORCID; Thomas Madura; Andrea MehnerORCID; Anthony Moffat; Maureen Y. Palmer; Gioia RauORCID; Noel D. RichardsonORCID; Gerd WeigeltORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. L23

The Lowest of the Low: Discovery of SN 2019gsc and the Nature of Faint Iax Supernovae

Shubham SrivastavORCID; Stephen J. SmarttORCID; Giorgos LeloudasORCID; Mark E. HuberORCID; Ken ChambersORCID; Daniele B. MalesaniORCID; Jens HjorthORCID; James H. Gillanders; A. Schultz; Stuart A. SimORCID; Katie AuchettlORCID; Johan P. U. FynboORCID; Christa GallORCID; Owen R. McBrienORCID; Armin Rest; Ken W. SmithORCID; Radoslaw Wojtak; David R. YoungORCID

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. L24

Multiwavelength Follow-up of the Hyperluminous Intermediate-mass Black Hole Candidate 3XMM J215022.4−055108

Dacheng LinORCID; Jay StraderORCID; Aaron J. RomanowskyORCID; Jimmy A. IrwinORCID; Olivier Godet; Didier BarretORCID; Natalie A. Webb; Jeroen HomanORCID; Ronald A. Remillard

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. L25

Could Quasar Lensing Time Delays Hint to a Core Component in Halos, Instead of H0 Tension?

Kfir Blum; Emanuele Castorina; Marko Simonović

<jats:title>Abstract</jats:title> <jats:p>The time delay measured between the images of gravitationally lensed quasars probes a combination of the angular diameter distance to the source-lens system and the mass density profile of the lens. Observational campaigns to measure such systems have reported a determination of the Hubble parameter <jats:italic>H</jats:italic> <jats:sub>0</jats:sub> that shows significant tension with independent determination based on the cosmic microwave background (CMB) and large-scale structure (LSS). We show that lens mass models that exhibit a cored component, coexisting with a cusp, probe a degenerate direction in the lens model parameter space, being an approximate mass sheet transformation. This family of lens models has not been considered by the cosmographic analyses. Once added to the model, the cosmographic error budget should become dependent on stellar kinematics uncertainties. We propose that a core component coexisting with a cusp could bring the lensing measurements of <jats:italic>H</jats:italic> <jats:sub>0</jats:sub> into accordance with the CMB/LSS value.</jats:p>

Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.

Pp. L27