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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

Tabla de contenidos

The Rest-frame H-band Luminosity Function of Red-sequence Galaxies in Clusters at 1.0 < z < 1.3

Jeffrey C. C. ChanORCID; Gillian WilsonORCID; Gregory RudnickORCID; Adam MuzzinORCID; Michael Balogh; Julie Nantais; Remco F. J. van der Burg; Pierluigi Cerulo; Andrea BivianoORCID; Michael C. CooperORCID; Ricardo DemarcoORCID; Ben ForrestORCID; Chris LidmanORCID; Allison NobleORCID; Lyndsay Old; Irene Pintos-CastroORCID; Andrew M. M. Reeves; Kristi A. WebbORCID; Howard K. C. Yee; Mohamed H. AbdullahORCID; Gabriella De LuciaORCID; Danilo MarchesiniORCID; Sean L. McGee; Mauro StefanonORCID; Dennis ZaritskyORCID

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

Pp. 119

PS18kh: A New Tidal Disruption Event with a Non-axisymmetric Accretion Disk

T. W.-S. HoloienORCID; M. E. HuberORCID; B. J. ShappeeORCID; M. EracleousORCID; K. AuchettlORCID; J. S. Brown; M. A. TuckerORCID; K. C. ChambersORCID; C. S. KochanekORCID; K. Z. Stanek; A. Rest; D. BersierORCID; R. S. Post; G. Aldering; K. A. Ponder; J. D. Simon; E. Kankare; D. Dong; G. Hallinan; N. A. ReddyORCID; R. L. SandersORCID; M. W. Topping; J. BulgerORCID; T. B. Lowe; E. A. MagnierORCID; A. S. B. Schultz; C. Z. WatersORCID; M. Willman; D. Wright; D. R. YoungORCID; Subo DongORCID; J. L. PrietoORCID; Todd A. Thompson; L. Denneau; H. FlewellingORCID; A. N. HeinzeORCID; S. J. SmarttORCID; K. W. Smith; B. StalderORCID; J. L. TonryORCID; H. Weiland; ; ;

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

Pp. 120

Direct Measurement of the Dissipation Rate Spectrum around Ion Kinetic Scales in Space Plasma Turbulence

Jiansen HeORCID; Die Duan; Tieyan WangORCID; Xingyu ZhuORCID; Wenya Li; Daniel VerscharenORCID; Xin Wang; Chuanyi TuORCID; Yuri KhotyaintsevORCID; Guan LeORCID; Jim Burch

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

Pp. 121

Statistics on the Magnetosheath Properties Related to Magnetopause Magnetic Reconnection

Hui ZhangORCID; Suiyan FuORCID; Zuyin Pu; Jianyong LuORCID; Jun ZhongORCID; Changbo Zhu; Weixing Wan; Libo LiuORCID

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

Pp. 122

The Effective Magnetic Field Decay of Radio Pulsars: Insights from the Statistical Properties of Their Spin Frequency's Second Derivatives

Yi XieORCID; Shuang-Nan ZhangORCID

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

Pp. 123

X-Rays from e ± Pair Halos

A. EungwanichayapantORCID; W. LuangtipORCID; W. Maithong; D. RuffoloORCID

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

Pp. 124

Tidal Interactions between Binary Stars Can Drive Lithium Production in Low-mass Red Giants

Andrew R. CaseyORCID; Anna Y. Q. HoORCID; Melissa Ness; David W. Hogg; Hans-Walter RixORCID; George C. AngelouORCID; Saskia HekkerORCID; Christopher A. Tout; John C. LattanzioORCID; Amanda I. KarakasORCID; Tyrone E. WoodsORCID; Adrian M. Price-WhelanORCID; Kevin C. SchlaufmanORCID

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

Pp. 125

The Sloan Digital Sky Survey Reverberation Mapping Project: Accretion Disk Sizes from Continuum Lags

Y. HomayouniORCID; Jonathan R. TrumpORCID; C. J. GrierORCID; Yue ShenORCID; D. A. Starkey; W. N. BrandtORCID; G. Fonseca Alvarez; P. B. HallORCID; Keith HorneORCID; Karen KinemuchiORCID; Jennifer I-Hsiu LiORCID; Ian D. McGreerORCID; Mouyuan SunORCID; L. C. HoORCID; D. P. Schneider

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

Pp. 126

Search for Intra-day Optical Variability in γ-Ray-loud Blazars S5 0716+714 and 3C 273

H. T. LiuORCID; Hai Cheng Feng; Y. X. Xin; J. M. Bai; S. K. Li; Fang Wang

<jats:title>Abstract</jats:title> <jats:p>We present the photometric observations of blazars S5 0716+714 and 3C 273 with high temporal resolution (30–60 s) in the <jats:italic>I</jats:italic> or <jats:italic>R</jats:italic> bands. The observations were performed with a 1.02 m optical telescope from 2007 March 7 to 2012 May 16. The <jats:italic>F</jats:italic>-test, one-way analysis of variance (ANOVA) test, and <jats:italic>z</jats:italic>-transformed discrete correlation function (ZDCF) cross-correlation zero lag test are used to search for intra-day variability (IDV). Four and five reliable IDVs survive three tests for S5 0716+714 and 3C 273, respectively. IDVs are found for S5 0716+714 and 3C 273. A flare on 2008 May 8 has Δ<jats:italic>I</jats:italic> ≈ 0.06 ± 0.01 mag in a duration of 0.54 hr for S5 0716+714. A flare on 2011 May 10 shows Δ<jats:italic>R</jats:italic> ≈ 0.05 ± 0.01 mag in a duration of 0.40 hr for 3C 273. Sharp dips appear on 2011 May 9 for 3C 273 and show Δ<jats:italic>R</jats:italic> ≈ 0.05 ± 0.01 mag. Under the assumptions that the IDV is tightly connected to black hole mass, <jats:italic>M</jats:italic> <jats:sub>•</jats:sub>, and that the flare durations are representative of the minimum characteristic timescales, we can estimate upper bounds to <jats:italic>M</jats:italic> <jats:sub>•</jats:sub>. In the case of the Kerr black holes, <jats:italic>M</jats:italic> <jats:sub>•</jats:sub> ≲ 10<jats:sup>8.91</jats:sup> <jats:italic>M</jats:italic> <jats:sub>⊙</jats:sub> and <jats:italic>M</jats:italic> <jats:sub>•</jats:sub> ≲ 10<jats:sup>9.02</jats:sup> <jats:italic>M</jats:italic> <jats:sub>⊙</jats:sub> are given for S5 0716+714 and 3C 273, respectively. These mass measurements are consistent with those measurements reported in the literature. Also, we discuss the origins of optical variations found in this work.</jats:p>

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

Pp. 155

EMPIRE: The IRAM 30 m Dense Gas Survey of Nearby Galaxies

María J. Jiménez-DonaireORCID; F. BigielORCID; A. K. LeroyORCID; A. UseroORCID; D. CormierORCID; J. Puschnig; M. GallagherORCID; A. KepleyORCID; A. BolattoORCID; S. García-BurilloORCID; A. HughesORCID; C. Kramer; J. PetyORCID; E. SchinnererORCID; A. Schruba; K. Schuster; F. WalterORCID

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

Pp. 127