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
The Star Formation History in the Solar Neighborhood as Told by Massive White Dwarfs
Jordi Isern
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L11
Intense C iv and He ii Emission inz∼ 0 Galaxies: Probing High-energy Ionizing Photons
Danielle A. Berg; John Chisholm; Dawn K. Erb; Richard Pogge; Alaina Henry; Grace M. Olivier
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L3
Discovery of An au-scale Excess in Millimeter Emission from the Protoplanetary Disk around TW Hya
Takashi Tsukagoshi; Takayuki Muto; Hideko Nomura; Ryohei Kawabe; Kazuhiro D. Kanagawa; Satoshi Okuzumi; Shigeru Ida; Catherine Walsh; Tom J. Millar; Sanemichi Z. Takahashi; Jun Hashimoto; Taichi Uyama; Motohide Tamura
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L8
On the Planetary Interpretation of Multiple Gaps and Rings in Protoplanetary Disks Seen By ALMA
Ryan Miranda; Roman R. Rafikov
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L9
Measuring the Delay Time Distribution of Binary Neutron Stars. I. Through Scaling Relations of the Host Galaxies of Gravitational-wave Events
Mohammadtaher Safarzadeh; Edo Berger
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L12
Measuring the Delay Time Distribution of Binary Neutron Stars. II. Using the Redshift Distribution from Third-generation Gravitational-wave Detectors Network
Mohammadtaher Safarzadeh; Edo Berger; Ken K. Y. Ng; Hsin-Yu Chen; Salvatore Vitale; Chris Whittle; Evan Scannapieco
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L13
Measuring the Delay Time Distribution of Binary Neutron Stars. III. Using the Individual Star Formation Histories of Gravitational-wave Event Host Galaxies in the Local Universe
Mohammadtaher Safarzadeh; Edo Berger; Joel Leja; Joshua S. Speagle
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L14
Spectral Diagnosis of Mg ii and Hα Lines during the Initial Stage of an M6.5 Solar Flare
Nengyi Huang; Yan Xu; Viacheslav M Sadykov; Ju Jing; Haimin Wang
<jats:title>Abstract</jats:title> <jats:p>Recent studies have shown special spectral properties during the initial stage of flare emissions, such as the enhanced absorption in He <jats:sc>i</jats:sc> 10830 Å line and a strong redshift in H<jats:italic>α</jats:italic>. Using the high-resolution imaging spectroscopic data obtained by the <jats:italic>Interface Region Imaging Spectrograph</jats:italic> (<jats:italic>IRIS</jats:italic>), we investigate the Mg <jats:sc>ii</jats:sc> emission lines during an M6.5 flare (SOL2015-06-22T18:23), which was well covered by the joint observation of <jats:italic>IRIS</jats:italic> and the Goode Solar Telescope at Big Bear Solar Observatory. On the leading edge of the propagating ribbon, Mg <jats:sc>ii</jats:sc> lines are characterized by blue-wing enhancement and strong broadening. On the other hand, redshifts in Mg <jats:sc>ii</jats:sc> and H<jats:italic>α</jats:italic> are found in the trailing areas of the flare ribbons. Numerical modeling, produced by combining RADYN and RH, suggests that the Mg <jats:sc>ii</jats:sc> line broadening is possibly caused by unresolved turbulence with velocities about 10 to 30 km s<jats:sup>−1</jats:sup>. The enhanced blue wing is likely due to a decrease of temperature and an increase of electron density, as consequences of electron precipitation. Based on the observations and simulation results, we discuss the possible response of the lower atmosphere to the electron precipitation, in terms of the evolution of temperature, electron density, and turbulence velocities.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L15
Using Surface Brightness Fluctuations to Study nearby Satellite Galaxy Systems: The Complete Satellite System of M101
Scott G. Carlsten; Rachael L. Beaton; Johnny P. Greco; Jenny E. Greene
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L16
Sub-threshold Binary Neutron Star Search in Advanced LIGO’s First Observing Run
Ryan Magee; Heather Fong; Sarah Caudill; Cody Messick; Kipp Cannon; Patrick Godwin; Chad Hanna; Shasvath Kapadia; Duncan Meacher; Siddharth R. Mohite; Debnandini Mukherjee; Alexander Pace; Surabhi Sachdev; Minori Shikauchi; Leo Singer
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. L17