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The Astrophysical Journal (ApJ)

Resumen/Descripción – provisto por la editorial en inglés
The Astrophysical Journal is an open access journal devoted to recent developments, discoveries, and theories in astronomy and astrophysics. Publications in ApJ constitute significant new research that is directly relevant to astrophysical applications, whether based on observational results or on theoretical insights or modeling.
Palabras clave – provistas por la editorial

astronomy; astrophysics

Disponibilidad
Institución detectada Período Navegá Descargá Solicitá
No detectada desde jul. 1995 / hasta dic. 2023 IOPScience

Información

Tipo de recurso:

revistas

ISSN impreso

0004-637X

ISSN electrónico

1538-4357

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

fisica

Ciencias físicas

Tabla de contenidos

doi: 10.3847/0004-637x/827/1/8

FRIENDS OF HOT JUPITERS. IV. STELLAR COMPANIONS BEYOND 50 au MIGHT FACILITATE GIANT PLANET FORMATION, BUT MOST ARE UNLIKELY TO CAUSE KOZAI–LIDOV MIGRATION

Henry NgoORCID; Heather A. Knutson; Sasha HinkleyORCID; Marta BryanORCID; Justin R. CreppORCID; Konstantin Batygin; Ian Crossfield; Brad Hansen; Andrew W. HowardORCID; John A. JohnsonORCID; Dimitri MawetORCID; Timothy D. MortonORCID; Philip S. MuirheadORCID; Ji WangORCID

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

Pp. 8

doi: 10.3847/0004-637x/827/1/9

PIXEL COLOR MAGNITUDE DIAGRAMS FOR SEMI-RESOLVED STELLAR POPULATIONS: THE STAR FORMATION HISTORY OF REGIONS WITHIN THE DISK AND BULGE OF M31

Charlie ConroyORCID; Pieter G. van Dokkum

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

Pp. 9

doi: 10.3847/0004-637x/827/1/10

IRON OPACITY BUMP CHANGES THE STABILITY AND STRUCTURE OF ACCRETION DISKS IN ACTIVE GALACTIC NUCLEI

Yan-Fei Jiang(姜燕飞)ORCID; Shane W. Davis; James M. Stone

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

Pp. 10

doi: 10.3847/0004-637x/827/1/11

SPACE-BASED MICROLENS PARALLAX OBSERVATION AS A WAY TO RESOLVE THE SEVERE DEGENERACY BETWEEN MICROLENS-PARALLAX AND LENS-ORBITAL EFFECTS

C. HanORCID; A. Udalski; C.-U. Lee; A. Gould; V. BozzaORCID; M. K. Szymański; I. Soszyński; J. SkowronORCID; P. Mróz; R. Poleski; P. PietrukowiczORCID; S. Kozłowski; K. Ulaczyk; Ł. Wyrzykowski; M. Pawlak; M. D. Albrow; S.-J. Chung; S.-L. Kim; S.-M. Cha; Y. K. Jung; D.-J. Kim; Y. Lee; B.-G. Park; Y.-H. Ryu; I.-G. Shin; J. C. YeeORCID; ;

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

Pp. 11

doi: 10.3847/0004-637x/827/1/12

HUBBLE SPACE TELESCOPEPROPER MOTION (HSTPROMO) CATALOGS OF GALACTIC GLOBULAR CLUSTERS. IV. KINEMATIC PROFILES AND AVERAGE MASSES OF BLUE STRAGGLER STARS

A. T. Baldwin; L. L. WatkinsORCID; R. P. van der MarelORCID; P. Bianchini; A. BelliniORCID; J. Anderson

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

Pp. 12

doi: 10.3847/0004-637x/827/1/13

TRANSIENT GALACTIC COSMIC-RAY MODULATION DURING SOLAR CYCLE 24: A COMPARATIVE STUDY OF TWO PROMINENT FORBUSH DECREASE EVENTS

L.-L. ZhaoORCID; H. ZhangORCID

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

Pp. 13

doi: 10.3847/0004-637x/827/1/14

ON THE THERMAL LINE EMISSION FROM THE OUTFLOWS IN ULTRALUMINOUS X-RAY SOURCES

Ya-Di Xu; Xinwu CaoORCID

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

Pp. 14

doi: 10.3847/0004-637x/827/1/15

COMPARING EXTENDED SYSTEM INTERACTIONS WITH MOTIONS IN SOFTENED POTENTIALS

Eric I. BarnesORCID

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

Pp. 15

doi: 10.3847/0004-637x/827/1/16

PITCH-ANGLE SCATTERING OF ENERGETIC CHARGED PARTICLES IN NEARLY CONSTANT MAGNITUDE MAGNETIC TURBULENCE

P. SunORCID; J. R. Jokipii; J. Giacalone

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

Pp. 16

doi: 10.3847/0004-637x/827/1/17

ABSOLUTE INTEGRAL CROSS SECTIONS FOR THE STATE-SELECTED ION–MOLECULE REACTION ${{{\rm{N}}}_{2}}^{+}({X}^{2}{{{\rm{\Sigma }}}_{{\rm{g}}}}^{+}$;v+= 0–2) + C2H2IN THE COLLISION ENERGY RANGE OF 0.03–10.00 eV

Yuntao Xu; Bo Xiong; Yih Chung Chang; C. Y. NgORCID

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

Pp. 17