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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

Accretion-driven Sources in Spatially Resolved Lyα Emitters

Benjamin Dittenber; M. S. OeyORCID; Edmund Hodges-KluckORCID; Elena Gallo; Matthew HayesORCID; Göran Östlin; Jens MelinderORCID

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

Pp. L12

Spontaneous Onset of Collisionless Magnetic Reconnection on an Electron Scale

Dongkuan Liu; San LuORCID; Quanming LuORCID; Weixing Ding; Shui Wang

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

Pp. L15

Upper Limit on the Dissipation of Gravitational Waves in Gravitationally Bound Systems

Abraham LoebORCID

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

Pp. L16

Fast Luminous Blue Transients in the Reionization Era and Beyond

Tomoki Terasaki; Daichi Tsuna; Toshikazu ShigeyamaORCID

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

Pp. L17

Probing Cosmic-Ray Transport with Radio Synchrotron Harps in the Galactic Center

Timon Thomas; Christoph PfrommerORCID; Torsten Enßlin

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

Pp. L18

No Massive Companion to the Coherent Radio-emitting M Dwarf GJ 1151

Benjamin J. S. PopeORCID; Megan BedellORCID; Joseph R. CallinghamORCID; Harish K. VedanthamORCID; Ignas A. G. SnellenORCID; Adrian M. Price-WhelanORCID; Timothy W. ShimwellORCID

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

Pp. L19

GW170817A as a Hierarchical Black Hole Merger

V. Gayathri; I. BartosORCID; Z. HaimanORCID; S. Klimenko; B. KocsisORCID; S. Márka; Y. Yang

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

Pp. L20

Excitation Sources of Oscillations in Solar Coronal Loops: A Multi-wavelength Analysis

Sandra M. Conde C.; Rekha JainORCID; Vera Jatenco-PereiraORCID

<jats:title>Abstract</jats:title> <jats:p>An investigation into the excitation sources of oscillations detected in a coronal loop structure is carried out using the images obtained with <jats:italic>Interface Region Imaging Spectrometer</jats:italic> (<jats:italic>IRIS</jats:italic>) and the Atmospheric Imaging Assembly (AIA) instrument on board the <jats:italic>Solar Dynamics Observatory</jats:italic> (<jats:italic>SDO</jats:italic>). A loop structure in the active region AR 11967 on 2014 January 28, oscillating in the vicinity of a strong eruption and an M3.6 class flare site, is clearly noticeable in <jats:italic>SDO</jats:italic>/AIA 171 Å images. We study in detail, the oscillations with detected periods between 4 and 13 minutes and their connection in <jats:italic>IRIS</jats:italic> SJI 1330 Å and <jats:italic>SDO</jats:italic>/AIA 1700 Å images; both of these wavelengths sample the lower parts of the solar atmosphere. The simultaneous presence of many oscillations in the region of interest in all three wavelength passbands suggest that these oscillations were excited in the lower-chromosphere–photosphere plasma connected to the loop structure and then propagated at higher heights. We further investigate the Doppler velocity measurements from the spectrograph snapshots in <jats:italic>IRIS</jats:italic> C <jats:sc>ii</jats:sc> 1336 Å, Si <jats:sc>iv</jats:sc> 1403 Å and Mg <jats:sc>ii</jats:sc> k 2796 Å. These show signatures of upflows in the vicinity of the loop structure’s endpoints estimated from 171 Å images. We suggest that some of the oscillations observed in AIA 171 Å have been triggered by plasma ejections and perturbations seen in the lower layers of the solar atmosphere. Based on the estimated phase speeds, the oscillations are likely to be slow magnetoacoustic in nature.</jats:p>

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

Pp. L21

13CH3OH Masers Associated With a Transient Phenomenon in a High-mass Young Stellar Object

Xi Chen; Andrej M. Sobolev; Shari L. BreenORCID; Zhi-Qiang Shen; Simon P. EllingsenORCID; Gordon C. MacLeod; Bin Li; Maxim A. Voronkov; Jane F. Kaczmarek; Jiangshui Zhang; Zhi-Yuan Ren; Jin Wang; Hendrik Linz; Todd R. HunterORCID; Crystal BroganORCID; Koichiro SugiyamaORCID; Ross A. BurnsORCID; Karl MentenORCID; Alberto Sanna; Bringfried Stecklum; Tomoya HirotaORCID; Kee-Tae KimORCID; James ChibuezeORCID; SP van den Heever

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

Pp. L22

Space Weathering Simulation with Low-energy Laser Irradiation of Murchison CM Chondrite for Reproducing Micrometeoroid Bombardments on C-type Asteroids

Moe MatsuokaORCID; Tomoki Nakamura; Takahiro Hiroi; Satoshi Okumura; Sho Sasaki

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

Pp. L23