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
Exemplary Merging Clusters: Weak-lensing and X-Ray Analysis of the Double Radio Relic, Merging Galaxy Clusters MACS J1752.0+4440 and ZWCL 1856.8+6616
Kyle Finner
; Kim HyeongHan; M. James Jee; David Wittman; William R. Forman; Reinout J. van Weeren; Nathan R. Golovich; William A. Dawson; Alexander Jones; Francesco de Gasperin; Christine Jones
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 72
Experimental and Computational Studies on the Physicochemical Behavior of Phosphine Induced by Reactions with H and D Atoms on Interstellar Ice Grains
Thanh Nguyen; Yasuhiro Oba; W. M. C. Sameera; Akira Kouchi; Naoki Watanabe
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 73
A Blueprint for the Milky Way’s Stellar Populations. III. Spatial Distributions and Population Fractions of Local Halo Stars
Deokkeun An; Timothy C. Beers
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 74
Numerical Models of Externally Irradiated Herbig–Haro Objects
D. Estrella-Trujillo; P. F. Velázquez; A. C. Raga; A. Esquivel
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 75
Toward a More Complex Understanding of Natal Super Star Clusters with Multiwavelength Observations
Allison H. Costa; Kelsey E. Johnson; Remy Indebetouw; Molly K. Finn; Crystal L. Brogan; Amy Reines
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 76
How Negative Energy and Kelvin–Helmholtz Instabilities Grow by Longitudinal Waves in Solar Atmospheric Jets
H. Pourjavadi; S. Vasheghani Farahani; Z. Fazel
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 77
Search for Neutrinos in Coincidence with Gravitational Wave Events from the LIGO–Virgo O3a Observing Run with the Super-Kamiokande Detector
K. Abe; C. Bronner; Y. Hayato; M. Ikeda; S. Imaizumi; J. Kameda; Y. Kanemura; Y. Kataoka; S. Miki; M. Miura; S. Moriyama; Y. Nagao; M. Nakahata; S. Nakayama; T. Okada; K. Okamoto; A. Orii; G. Pronost; H. Sekiya; M. Shiozawa; Y. Sonoda; Y. Suzuki; A. Takeda; Y. Takemoto; A. Takenaka; H. Tanaka; S. Watanabe; T. Yano; S. Han; T. Kajita; K. Okumura; T. Tashiro; R. Wang; J. Xia; G. D. Megias; D. Bravo-Berguño; L. Labarga; Ll. Marti; B. Zaldivar; B. W. Pointon; F. d. M. Blaszczyk; E. Kearns; J. L. Raaf; J. L. Stone; L. Wan; T. Wester; J. Bian; N. J. Griskevich; W. R. Kropp; S. Locke; S. Mine; M. B. Smy; H. W. Sobel; V. Takhistov; P. Weatherly; J. Hill; J. Y. Kim; I. T. Lim; R. G. Park; B. Bodur; K. Scholberg; C. W. Walter; L. Bernard; A. Coffani; O. Drapier; S. El Hedri; A. Giampaolo; M. Gonin; Th. A. Mueller; P. Paganini; B. Quilain; T. Ishizuka; T. Nakamura; J. S. Jang; J. G. Learned; L. H. V. Anthony; D. G. R. Martin; A. A. Sztuc; Y. Uchida; V. Berardi; M. G. Catanesi; E. Radicioni; N. F. Calabria; L. N. Machado; G. De Rosa; G. Collazuol; F. Iacob; M. Lamoureux; N. Ospina; L. Ludovici; Y. Maekawa; Y. Nishimura; S. Cao; M. Friend; T. Hasegawa; T. Ishida; M. Jakkapu; T. Kobayashi; T. Matsubara; T. Nakadaira; K. Nakamura; Y. Oyama; K. Sakashita; T. Sekiguchi; T. Tsukamoto; Y. Kotsar; Y. Nakano; H. Ozaki; T. Shiozawa; A. T. Suzuki; Y. Takeuchi; S. Yamamoto; A. Ali; Y. Ashida; J. Feng; S. Hirota; T. Kikawa; M. Mori; T. Nakaya; R. A. Wendell; K. Yasutome; P. Fernandez; N. McCauley; P. Mehta; A. Pritchard; K. M. Tsui; Y. Fukuda; Y. Itow; H. Menjo; T. Niwa; K. Sato; M. Tsukada; P. Mijakowski; J. Jiang; C. K. Jung; C. Vilela; M. J. Wilking; C. Yanagisawa; K. Hagiwara; M. Harada; T. Horai; H. Ishino; S. Ito; Y. Koshio; H. Kitagawa; W. Ma; N. Piplani; S. Sakai; Y. Kuno; G. Barr; D. Barrow; L. Cook; A. Goldsack; S. Samani; C. Simpson; D. Wark; F. Nova; T. Boschi; F. Di Lodovico; J. Migenda; S. Molina Sedgwick; M. Taani; S. Zsoldos; J. Y. Yang; S. J. Jenkins; M. Malek; J. M. McElwee; O. Stone; M. D. Thiesse; L. F. Thompson; H. Okazawa; S. B. Kim; I. Yu; K. Nishijima; M. Koshiba; K. Iwamoto; Y. Nakajima; N. Ogawa; M. Yokoyama; K. Martens; M. R. Vagins; S. Izumiyama; M. Kuze; M. Tanaka; T. Yoshida; M. Inomoto; M. Ishitsuka; H. Ito; R. Matsumoto; K. Ohta; M. Shinoki; J. F. Martin; H. A. Tanaka; T. Towstego; R. Akutsu; M. Hartz; A. Konaka; P. de Perio; N. W. Prouse; S. Chen; B. D. Xu; M. Posiadala-Zezula; D. Hadley; B. Richards; B. Jamieson; J. Walker; A. Minamino; K. Okamoto; G. Pintaudi; S. Sano; R. Sasaki; A. K. Ichikawa; K. Nakamura
<jats:title>Abstract</jats:title> <jats:p>The Super-Kamiokande detector can be used to search for neutrinos in time coincidence with gravitational waves detected by the LIGO–Virgo Collaboration (LVC). Both low-energy (7–100 MeV) and high-energy (0.1–10<jats:sup>5</jats:sup> GeV) samples were analyzed in order to cover a very wide neutrino spectrum. Follow-ups of 36 (out of 39) gravitational waves reported in the GWTC-2 catalog were examined; no significant excess above the background was observed, with 10 (24) observed neutrinos compared with 4.8 (25.0) expected events in the high-energy (low-energy) samples. A statistical approach was used to compute the significance of potential coincidences. For each observation, <jats:italic>p</jats:italic>-values were estimated using neutrino direction and LVC sky map; the most significant event (GW190602_175927) is associated with a post-trial <jats:italic>p</jats:italic>-value of 7.8% (1.4<jats:italic>σ</jats:italic>). Additionally, flux limits were computed independently for each sample and by combining the samples. The energy emitted as neutrinos by the identified gravitational wave sources was constrained, both for given flavors and for all flavors assuming equipartition between the different flavors, independently for each trigger and by combining sources of the same nature.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 78
Prior Probability Distributions of Neutron Star Crust Models
Lauren E. Balliet; William G. Newton; Sarah Cantu; Srdan Budimir
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 79
Search for Long-duration Gravitational-wave Signals Associated with Magnetar Giant Flares
A. Macquet; M. A. Bizouard; E. Burns; N. Christensen; M. Coughlin; Z. Wadiasingh; G. Younes
<jats:title>Abstract</jats:title> <jats:p>Magnetar giant flares are rare and highly energetic phenomena observed in the transient sky whose emission mechanisms are still not fully understood. Depending on the nature of the excited modes of the magnetar, they are also expected to emit gravitational waves (GWs), which may bring unique information about the dynamics of the excitation. A few magnetar giant flares have been proposed to be associated with short gamma-ray bursts. In this paper we use a new gravitational-wave search algorithm to revisit the possible emission of GWs from four magnetar giant flares within 5 Mpc. While no gravitational-wave signals were observed, we discuss the future prospects of detecting signals with more sensitive gravitational-wave detectors. In particular, we show that galactic magnetar giant flares that emit at least 1% of their electromagnetic energy as GWs could be detected during the planned observing run of the LIGO and Virgo detectors at design sensitivity, with even better prospects for third-generation detectors.</jats:p>
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 80
Gas-phase Formation of Cationic Fullerene/Amino Acid Clusters: Evidence for the “Magic Number” Chemical Reactivity of Fullerene Cations
Xiaoyi Hu; Deping Zhang; Yuanyuan Yang; Yang Chen; Liping Qin; Junfeng Zhen
Palabras clave: Space and Planetary Science; Astronomy and Astrophysics.
Pp. 81