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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

Learning How to Surf: Reconstructing the Propagation and Origin of Gravitational Waves with Gaussian Processes

Guadalupe Cañas-HerreraORCID; Omar ContigianiORCID; Valeri VardanyanORCID

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

Pp. 20

Following the Lithium: Tracing Li-bearing Molecules across Age, Mass, and Gravity in Brown Dwarfs

Ehsan Gharib-NezhadORCID; Mark S. MarleyORCID; Natasha E. BatalhaORCID; Channon VisscherORCID; Richard S. FreedmanORCID; Roxana E. LupuORCID

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

Pp. 21

Coronal Hole Detection and Open Magnetic Flux

Jon A. LinkerORCID; Stephan G. HeinemannORCID; Manuela TemmerORCID; Mathew J. OwensORCID; Ronald M. CaplanORCID; Charles N. Arge; Eleanna AsvestariORCID; Veronique DelouilleORCID; Cooper DownsORCID; Stefan J. HofmeisterORCID; Immanuel C. JebarajORCID; Maria S. MadjarskaORCID; Rui F. PintoORCID; Jens PomoellORCID; Evangelia SamaraORCID; Camilla ScoliniORCID; Bojan Vršnak

<jats:title>Abstract</jats:title> <jats:p>Many scientists use coronal hole (CH) detections to infer open magnetic flux. Detection techniques differ in the areas that they assign as open, and may obtain different values for the open magnetic flux. We characterize the uncertainties of these methods, by applying six different detection methods to deduce the area and open flux of a near-disk center CH observed on 2010 September 19, and applying a single method to five different EUV filtergrams for this CH. Open flux was calculated using five different magnetic maps. The standard deviation (interpreted as the uncertainty) in the open flux estimate for this CH ≈ 26%. However, including the variability of different magnetic data sources, this uncertainty almost doubles to 45%. We use two of the methods to characterize the area and open flux for all CHs in this time period. We find that the open flux is greatly underestimated compared to values inferred from in situ measurements (by 2.2–4 times). We also test our detection techniques on simulated emission images from a thermodynamic MHD model of the solar corona. We find that the methods overestimate the area and open flux in the simulated CH, but the average error in the flux is only about 7%. The full-Sun detections on the simulated corona underestimate the model open flux, but by factors well below what is needed to account for the missing flux in the observations. Under-detection of open flux in coronal holes likely contributes to the recognized deficit in solar open flux, but is unlikely to resolve it.</jats:p>

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

Pp. 21

The Unusual Weak-line Quasar PG1407+265 and Its Foreground z ∼ 0.7 X-Ray Cluster

Jonathan C. McDowellORCID; Aneta SiemiginowskaORCID; Matthew AshbyORCID; Katherine BlundellORCID; Luigi C. Gallo

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

Pp. 22

The Sizes of Quasar Host Galaxies in the Hyper Suprime-Cam Subaru Strategic Program

Junyao LiORCID; John D. SilvermanORCID; Xuheng DingORCID; Michael A. StraussORCID; Andy GouldingORCID; Simon BirrerORCID; Hassen M. YesufORCID; Yongquan XueORCID; Lalitwadee KawinwanichakijORCID; Yoshiki Matsuoka; Yoshiki TobaORCID; Tohru NagaoORCID; Malte SchrammORCID; Kohei InayoshiORCID

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

Pp. 22

Probing Jets from Young Embedded Sources: Clues from HST Near-IR [Fe ii] Images

Jessica ErkalORCID; Brunella NisiniORCID; Deirdre CoffeyORCID; Francesca BacciottiORCID; Patrick HartiganORCID; Simone AntoniucciORCID; Teresa GianniniORCID; Jochen EislöffelORCID; Carlo Felice ManaraORCID

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

Pp. 23

Galaxy Properties at the Faint End of the H i Mass Function

Kristen B. W. McQuinnORCID; Anjana K. Telidevara; Jackson Fuson; Elizabeth A. K. AdamsORCID; John M. CannonORCID; Evan D. SkillmanORCID; Andrew E. DolphinORCID; Martha P. HaynesORCID; Katherine L. RhodeORCID; John. J. SalzerORCID; Riccardo Giovanelli; Alex J. R. Gordon

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

Pp. 23

Detecting Neutrino Mass by Combining Matter Clustering, Halos, and Voids

Adrian E. BayerORCID; Francisco Villaescusa-NavarroORCID; Elena MassaraORCID; Jia LiuORCID; David N. SpergelORCID; Licia VerdeORCID; Benjamin D. WandeltORCID; Matteo VielORCID; Shirley Ho

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

Pp. 24

Fermi-LAT Detection of GeV γ-Ray Emission from the Type Ia Supernova Remnant G272.2–3.2

Yunchuan XiangORCID; Zejun Jiang

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

Pp. 24

The Stellar Mass in and around Isolated Central Galaxies: Connections to the Total Mass Distribution through Galaxy–Galaxy Lensing in the Hyper Suprime-Cam Survey

Wenting WangORCID; Xiangchong LiORCID; Jingjing ShiORCID; Jiaxin HanORCID; Naoki Yasuda; Yipeng JingORCID; Surhud MoreORCID; Masahiro TakadaORCID; Hironao Miyatake; Atsushi J. NishizawaORCID

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

Pp. 25