Catálogo de publicaciones - revistas
Título de Acceso Abierto
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
Cobertura temática
Tabla de contenidos
Flatness without CMB: The Entanglement of Spatial Curvature and Dark Energy Equation of State
Haoting Xu; Zhiqi Huang; Zhenjie Liu; Haitao Miao
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 107
Anisotropic Structure of Synchrotron Polarization
Hyeseung Lee
; Jungyeon Cho; A. Lazarian
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 108
Theoretical Transmission Spectra of Exoplanet Atmospheres with Hydrocarbon Haze: Effect of Creation, Growth, and Settling of Haze Particles. II. Dependence on UV Irradiation Intensity, Metallicity, C/O Ratio, Eddy Diffusion Coefficient, and Temperature
Yui Kawashima; Masahiro Ikoma
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 109
SPIRITS Catalog of Infrared Variables: Identification of Extremely Luminous Long Period Variables
V. R. Karambelkar; S. M. Adams; P. A. Whitelock; M. M. Kasliwal; J. E. Jencson; M. L. Boyer; S. R. Goldman; F. Masci; A. M. Cody; J. Bally; H. E. Bond; R. D. Gehrz; M. Parthasarathy; R. M. Lau;
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 110
Data-optimized Coronal Field Model. I. Proof of Concept
K. Dalmasse; A. Savcheva; S. E. Gibson; Y. Fan; D. W. Nychka; N. Flyer; N. Mathews; E. E. DeLuca
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 111
Multiline Observations of Molecular Bullets from a High-mass Protostar
Yu Cheng; Keping Qiu; Qizhou Zhang; Friedrich Wyrowski; Karl Menten; Rolf Güsten
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 112
Investigation of a Vorticity-preserving Scheme for the Euler Equations
Darryl Seligman; Karim Shariff
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 113
TRAO Survey of Nearby Filamentary Molecular Clouds, the Universal Nursery of Stars (TRAO FUNS). I. Dynamics and Chemistry of L1478 in the California Molecular Cloud
Eun Jung Chung; Chang Won Lee; Shinyoung Kim; Gwanjeong Kim; Paola Caselli; Mario Tafalla; Philip C. Myers; Archana Soam; Tie Liu; Maheswar Gopinathan; Miryang Kim; Kyoung Hee Kim; Woojin Kwon; Hyunwoo Kang; Changhoon Lee
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 114
Magnetic Activity and Orbital Period Study for the Short-period RS CVn–type Eclipsing Binary DV Psc
Qing-feng Pi; Li-yun Zhang; Shao-lan Bi; Xianming L. Han; Hong-peng Lu; Qiang Yue; Liu Long; Yan Yan
<jats:title>Abstract</jats:title> <jats:p>Using 27 sets of new multiband photometry light curves acquired from our long-term photometric campaign carried out in the last 5 yr and high-resolution spectroscopic data from seven nights, we analyzed the physical mechanisms of period variation, starspot cycle, optical flares, and chromospheric activities of the eclipsing binary DV Psc. Our updated <jats:italic>O</jats:italic> − <jats:italic>C</jats:italic> diagram covering a period of approximately 20 yr shows an oscillation in its orbital period. This variations might be caused by a third body with an orbital period of 14.58 ± 0.28 yr. There are two active regions of starspots at longitude belts of about 90° and 270°. We obtained its starspot cycles with periods of 3.60 ± 0.03 yr and 3.42 ± 0.02 yr at about 90° and 270°, respectively. Moreover, the magnitude difference of Max. I–Max. II shows cyclic oscillation of 5.15 ± 0.01 yr. During our decade long photometric campaign, we observed DV Psc a total of 326.4 hr, detected 18 outbursts (12 of them have never been reported) with flare energies in the range of (6.62–1106.85) × 10<jats:sup>24</jats:sup> J. The slope of the relationship between the phase of the max flare and spots is 0.842 ± 0.083, implying a correlation between spots and flares. We discovered evidence for a correlation between the rotation period and the activity cycle for the short-period eclipsing binaries. Our high-resolution spectroscopic observations of DV Psc show obvious emissions above continuum in the H<jats:sub> <jats:italic>α</jats:italic> </jats:sub> line and small self-reversal emissions of the Ca <jats:sc>ii</jats:sc> IRT lines.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 75
Discovery of a New Class I Methanol Maser Transition at 266.8 GHz
Xi Chen; Simon P. Ellingsen; Zhi-Yuan Ren; Andrej M. Sobolev; Sergey Parfenov; Zhi-Qiang Shen
<jats:title>Abstract</jats:title> <jats:p>We report the detection of a new class I methanol maser candidate from the 5<jats:sub>2</jats:sub>−4<jats:sub>1</jats:sub> <jats:italic>E</jats:italic> transition (266.8 GHz). This methanol transition has been detected toward a nearby high-mass star-forming region G352.630-1.067 (distance ∼0.7 kpc), in Submillimeter Array (SMA) observations. The new candidate transition has a similar spatial distribution as the 4<jats:sub>2</jats:sub>−3<jats:sub>1</jats:sub> <jats:italic>E</jats:italic> (218.4 GHz) and 8<jats:sub>−1</jats:sub>−7<jats:sub>0</jats:sub> <jats:italic>E</jats:italic> (229.7 GHz) transitions, which are known class I maser transitions. Thermal methanol emission in this source is confined to a central hot core, while the three class I maser transitions are detected in two additional regions. These two maser-only emission regions are clearly associated with shocked gas traced by 2 <jats:italic>μ</jats:italic>m <jats:italic>Ks</jats:italic>-band and thermal <jats:italic>v</jats:italic> = 0, <jats:italic>J</jats:italic> = 5−4 SiO molecular emission. In contrast to the thermal methanol emission from the hot core, the three class I maser transitions show an positive trend in the rotation diagram for the two maser regions. Large velocity gradient modeling of the 266.8, 218.4, and 229.7 GHz transitions shows that the 266.8 GHz transition can be a maser for a wide range of conditions. The intensity ratios for the three methanol transitions detected in maser regions can be reproduced under conditions that are typical for class I methanol maser sites. These facts all support the hypothesis that the detected emission from the 266.8 GHz methanol (5<jats:sub>2</jats:sub>−4<jats:sub>1</jats:sub> <jats:italic>E</jats:italic>) transition is masing.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 90