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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

PLANETS AROUND THE K-GIANTS BD+20 274 AND HD 219415

S. Gettel; A. Wolszczan; A. Niedzielski; G. Nowak; M. Adamów; P. Zieliński; G. Maciejewski

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

Pp. 53

BROADBAND SPECTRAL INVESTIGATIONS OF SGR J1550–5418 BURSTS

Lin Lin; Ersin Göğüş; Matthew G. Baring; Jonathan Granot; Chryssa Kouveliotou; Yuki Kaneko; Alexander van der Horst; David Gruber; Andreas von Kienlin; George Younes; Anna L. Watts; Neil Gehrels

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

Pp. 54

FRACTIONAL AMPLITUDE OF KILOHERTZ QUASI-PERIODIC OSCILLATION FROM 4U 1728-34: EVIDENCE OF DECLINE AT HIGHER ENERGIES

Arunava Mukherjee; Sudip Bhattacharyya

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

Pp. 55

LARGE-MASS NEUTRON STARS WITH HYPERONIZATION

Wei-Zhou Jiang; Bao-An Li; Lie-Wen Chen

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

Pp. 56

ENERGY RELAXATION OF HELIUM ATOMS IN ASTROPHYSICAL GASES

N. R. Lewkow; V. Kharchenko; P. Zhang

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

Pp. 57

CHEMISTRY IN DISKS. VII. FIRST DETECTION OF HC3N IN PROTOPLANETARY DISKS

Edwige Chapillon; Anne Dutrey; Stéphane Guilloteau; Vincent Piétu; Valentine Wakelam; Franck Hersant; Fréderic Gueth; Thomas Henning; Ralf Launhardt; Katharina Schreyer; Dmitry Semenov

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

Pp. 58

SLOW RISE AND PARTIAL ERUPTION OF A DOUBLE-DECKER FILAMENT. I. OBSERVATIONS AND INTERPRETATION

Rui Liu; Bernhard Kliem; Tibor Török; Chang Liu; Viacheslav S. Titov; Roberto Lionello; Jon A. Linker; Haimin Wang

<jats:title>ABSTRACT</jats:title> <jats:p>We study an active-region dextral filament that was composed of two branches separated in height by about 13 Mm, as inferred from three-dimensional reconstruction by combining <jats:italic>SDO</jats:italic> and <jats:italic>STEREO-B</jats:italic> observations. This “double-decker” configuration sustained for days before the upper branch erupted with a <jats:italic>GOES</jats:italic>-class M1.0 flare on 2010 August 7. Analyzing this evolution, we obtain the following main results. (1) During the hours before the eruption, filament threads within the lower branch were observed to intermittently brighten up, lift upward, and then merge with the upper branch. The merging process contributed magnetic flux and current to the upper branch, resulting in its quasi-static ascent. (2) This transfer might serve as the key mechanism for the upper branch to lose equilibrium by reaching the limiting flux that can be stably held down by the overlying field or by reaching the threshold of the torus instability. (3) The erupting branch first straightened from a reverse S shape that followed the polarity inversion line and then writhed into a forward S shape. This shows a transfer of left-handed helicity in a sequence of writhe–twist–writhe. The fact that the initial writhe is converted into the twist of the flux rope excludes the helical kink instability as the trigger process of the eruption, but supports the occurrence of the instability in the main phase, which is indeed indicated by the very strong writhing motion. (4) A hard X-ray sigmoid, likely of coronal origin, formed in the gap between the two original filament branches in the impulsive phase of the associated flare. This supports a model of transient sigmoids forming in the vertical flare current sheet. (5) Left-handed magnetic helicity is inferred for both branches of the dextral filament. (6) Two types of force-free magnetic configurations are compatible with the data, a double flux rope equilibrium and a single flux rope situated above a loop arcade.</jats:p>

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

Pp. 59

CHEMISTRY IN INFRARED DARK CLOUD CLUMPS: A MOLECULAR LINE SURVEY AT 3 mm

Patricio Sanhueza; James M. Jackson; Jonathan B. Foster; Guido Garay; Andrea Silva; Susanna C. Finn

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

Pp. 60

ON THE EXISTENCE OF “RADIO THERMALLY ACTIVE” GALACTIC SUPERNOVA REMNANTS

D. Onić; D. Urošević; B. Arbutina; D. Leahy

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

Pp. 61

ROSSBY WAVE INSTABILITY AT DEAD ZONE BOUNDARIES IN THREE-DIMENSIONAL RESISTIVE MAGNETOHYDRODYNAMICAL GLOBAL MODELS OF PROTOPLANETARY DISKS

Wladimir Lyra; Mordecai-Mark Mac Low

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

Pp. 62