Catálogo de publicaciones - revistas
Título de Acceso Abierto
The Astrophysical Journal Supplement (ApJS)
Resumen/Descripción – provisto por la editorial en inglés
The Astrophysical Journal Supplement is an open access journal publishing significant articles containing extensive data or calculations. ApJS also supports Special Issues, collections of thematically related papers published simultaneously in a single volume.Palabras clave – provistas por la editorial
astronomy; astrophysics
Disponibilidad
| Institución detectada | Período | Navegá | Descargá | Solicitá |
|---|---|---|---|---|
| No detectada | desde dic. 1996 / hasta dic. 2023 | IOPScience |
Información
Tipo de recurso:
revistas
ISSN impreso
0067-0049
ISSN electrónico
1538-4365
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
Modeling Dense Star Clusters in the Milky Way and Beyond with the CMC Cluster Catalog
Kyle Kremer
; Claire S. Ye; Nicholas Z. Rui; Newlin C. Weatherford; Sourav Chatterjee; Giacomo Fragione; Carl L. Rodriguez; Mario Spera; Frederic A. Rasio
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 48
Multicolor Optical Monitoring of the Blazar S5 0716+714 from 2017 to 2019
Dingrong Xiong; Jinming Bai; Junhui Fan; Dahai Yan; Minfeng Gu; Xuliang Fan; Jirong Mao; Nan Ding; Rui Xue; Weimin Yi
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 49
Physical Parameters of Late-type Contact Binaries in the Northern Catalina Sky Survey
Weijia Sun; Xiaodian Chen; Licai Deng; Richard de Grijs
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 50
The Gravitational Instability of Adiabatic Filaments
Eric R. Coughlin; C. J. Nixon
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 51
Relativistic MR-MP Energy Levels for K-like Fe
Juan A. Santana; Yasuyuki Ishikawa; Peter Beiersdorfer
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 52
Radio Sources Associated with Optical Galaxies and Having Unresolved or Extended Morphologies (ROGUE). I. A Catalog of SDSS Galaxies with FIRST Core Identifications
Dorota Kozieł-Wierzbowska; Arti Goyal; Natalia Żywucka
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 53
2SXPS: An Improved and Expanded Swift X-Ray Telescope Point-source Catalog
P. A. Evans; K. L. Page; J. P. Osborne; A. P. Beardmore; R. Willingale; D. N. Burrows; J. A. Kennea; M. Perri; M. Capalbi; G. Tagliaferri; S. B. Cenko
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 54
An Accurate, Extensive, and Practical Line List of Methane for the HITEMP Database
Robert J. Hargreaves; Iouli E. Gordon; Michael Rey; Andrei V. Nikitin; Vladimir G. Tyuterev; Roman V. Kochanov; Laurence S. Rothman
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 55
Single-pulse Detection Algorithms for Real-time Fast Radio Burst Searches Using GPUs
Karel Adámek; Wesley Armour
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 56
Compact Bright Radio-loud AGNs. III. A Large VLBA Survey at 43 GHz
X.-P. Cheng; T. An; S. Frey; X.-Y. Hong; X. He; K. I. Kellermann; M. L. Lister; B.-Q. Lao; X.-F. Li; P. Mohan; J. Yang; X.-C. Wu; Z.-L. Zhang; Y.-K. Zhang; W. Zhao
<jats:title>Abstract</jats:title> <jats:p>We present the results from the 43 GHz Very Long Baseline Array (VLBA) observations of 124 compact radio-loud active galactic nuclei (AGNs) that were conducted between 2014 November and 2016 May. The typical dimensions of the restoring beam in each image are about 0.5 mas × 0.2 mas. The highest resolution of 0.2 mas corresponds to a physical size of 0.02 pc for the lowest redshift source in the sample. The 43 GHz very long baseline interferometry (VLBI) images of 97 AGNs are presented for the first time. We study the source compactness on milliarcsecond and submilliarcsecond scales, and suggest that 95 sources in our sample are suitable for future space VLBI observations. By analyzing our data supplemented with other VLBA AGN surveys from the literature, we find that the core brightness temperature increases with increasing frequency below a break frequency ∼7 GHz, and decreases between ∼7 and 240 GHz but increases again above 240 GHz in the rest frame of the sources. This indicates that the synchrotron opacity changes from optically thick to thin. We also find a strong statistical correlation between radio and <jats:italic>γ</jats:italic>-ray flux densities. Our correlation is tighter than those in the literature derived from lower-frequency VLBI data, suggesting that the <jats:italic>γ</jats:italic>-ray emission is produced more cospatially with the 43 GHz VLBA core emission. This correlation can also be extrapolated to the unbeamed AGN population, implying that a universal <jats:italic>γ</jats:italic>-ray production mechanism might be at work for all types of AGNs.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 57