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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

Hydrodynamical Models of Protoplanetary Nebulae Including the Photoionization of the Central Star

D. Estrella-TrujilloORCID; L. Hernández-Martínez; P. F. VelázquezORCID; A. EsquivelORCID; A. C. RagaORCID

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

Pp. 29

Constraining the Tail End of Reionization Using Lyα Transmission Spikes

Enrico GaraldiORCID; Nickolay Y. Gnedin; Piero MadauORCID

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

Pp. 31

Unbiased Cosmological Parameter Estimation from Emission-line Surveys with Interlopers

Henry S. Grasshorn GebhardtORCID; Donghui JeongORCID; Humna AwanORCID; Joanna S. BridgeORCID; Robin CiardulloORCID; Daniel Farrow; Karl Gebhardt; Gary J. Hill; Eiichiro KomatsuORCID; Mallory MolinaORCID; Ana Paulino-Afonso; Shun Saito; Donald P. Schneider; Greg ZeimannORCID

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

Pp. 32

The Origins of Protostellar Core Angular Momenta

Aleksandra KuznetsovaORCID; Lee HartmannORCID; Fabian HeitschORCID

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

Pp. 33

Detection of a White Dwarf Companion to a Blue Straggler Star in the Outskirts of Globular Cluster NGC 5466 with the Ultraviolet Imaging Telescope (UVIT)

Snehalata SahuORCID; Annapurni Subramaniam; Mirko Simunovic; J. Postma; Patrick Côté; N. Kameswera RaoORCID; Aaron M. GellerORCID; Nathan Leigh; Michael SharaORCID; Thomas H. PuziaORCID; Peter B. StetsonORCID

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

Pp. 34

Evidence for a Young Stellar Population in Nearby Type 1 Active Galaxies

Minjin KimORCID; Luis C. HoORCID

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

Pp. 35

Moving Groups as the Origin of the Vertical Phase Space Spiral in the Solar Neighborhood

Tatiana A. MichtchenkoORCID; Douglas A. BarrosORCID; Angeles Pérez-VillegasORCID; Jacques R. D. LépineORCID

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

Pp. 36

Possible Evidence for Cosmic-Ray Acceleration in the Type Ia SNR RCW 86: Spatial Correlation between TeV Gamma-Rays and Interstellar Atomic Protons

H. SanoORCID; G. RowellORCID; E. M. Reynoso; I. Jung-Richardt; Y. YamaneORCID; T. Nagaya; S. YoshiikeORCID; K. HayashiORCID; K. ToriiORCID; N. MaxtedORCID; I. Mitsuishi; T. Inoue; S. InutsukaORCID; H. Yamamoto; K. TachiharaORCID; Y. Fukui

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

Pp. 37

Noncircular Motions in the Outer Perseus Spiral Arm

Nobuyuki Sakai; Mark J. ReidORCID; Karl M. MentenORCID; Andreas BrunthalerORCID; Thomas M. DameORCID

<jats:title>Abstract</jats:title> <jats:p>We report measurements of parallax and proper motion for five 6.7 GHz methanol maser sources in the outer regions of the Perseus arm as part of the BeSSeL Survey of the Galaxy. By combining our results with previous astrometric results, we determine an average spiral arm pitch angle of 9.°2 ± 1.°5 and an arm width of 0.39 kpc for this spiral arm. For sources on the interior side of the Perseus arm, we find on average a radial inward motion in the Galaxy of 13.3 ± 5.4 km s<jats:sup>−1</jats:sup> and counter to Galactic rotation of 6.2 ± 3.2 km s<jats:sup>−1</jats:sup>. These characteristics are consistent with models for spiral arm formation that involve gas entering an arm to be shocked and then to form stars. However, similar data for other spiral arms do not show similar characteristics.</jats:p>

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

Pp. 30

Dicarbon Formation in Collisions of Two Carbon Atoms

James F. BabbORCID; R. T. SmythORCID; B. M. McLaughlinORCID

<jats:title>Abstract</jats:title> <jats:p>Radiative association cross sections and rates are computed, using a quantum approach, for the formation of C<jats:sub>2</jats:sub> molecules (dicarbon) during the collision of two ground-state C(<jats:sup>3</jats:sup> <jats:italic>P</jats:italic>) atoms. We find that transitions originating in the C <jats:sup>1</jats:sup>Π<jats:sub> <jats:italic>g</jats:italic> </jats:sub>, d <jats:sup>3</jats:sup>Π<jats:sub> <jats:italic>g</jats:italic> </jats:sub>, and 1 <jats:sup>5</jats:sup>Π<jats:sub> <jats:italic>u</jats:italic> </jats:sub> states are the main contributors to the process. The results are compared and contrasted with previous results obtained from a semiclassical approximation. New ab initio potential curves and transition dipole moment functions have been obtained for the present work using the multi-reference configuration interaction approach with the Davidson correction (MRCI+Q) and aug-cc-pCV5Z basis sets, substantially increasing the available molecular data on dicarbon. Applications of the current computations to various astrophysical environments and laboratory studies are briefly discussed, focusing on these rates.</jats:p>

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

Pp. 38