Search Publications

Very Long Baseline Array Observations of Parsec-scale Radio Emission in Dual Active Galactic Nuclei
DOI: 10.3847/1538-4357/ad463b Bibcode: 2024ApJ...969...36X

Ho, Luis C.; Zhang, Ming; An, Tao +11 more

It is believed that dual active galactic nuclei (AGN) form during galaxy mergers. Studying dual-AGN emission can provide valuable insights into galaxy merging and evolution. To investigate parsec-scale radio emission properties, we observed eight radio components of four selected dual-AGN systems using the Very Long Baseline Array (VLBA) at 5 GHz …

2024 The Astrophysical Journal
Gaia 0
Study of Plasma Heating Processes in a Coronal Mass Ejection–driven Shock Sheath Region Observed with the Metis Coronagraph
DOI: 10.3847/1538-4357/ad26fb Bibcode: 2024ApJ...964...15F

Susino, Roberto; Fineschi, Silvano; Stangalini, Marco +25 more

On 2021 September 28, a C1.6 class flare occurred in active region NOAA 12871, located approximately at 27°S and 51°W on the solar disk with respect to Earth's point of view. This event was followed by a partial halo coronal mass ejection (CME) that caused the deflection of preexisting coronal streamer structures, as observed in visible-light coro…

2024 The Astrophysical Journal
SolarOrbiter 0
Fluorine Abundances in Local Stellar Populations
DOI: 10.3847/1538-3881/ad393a Bibcode: 2024AJ....167..291B

Grisoni, V.; Brady, K. E.; Pilachowski, C. A. +2 more

We present the first fluorine measurements in 12 normal K giants belonging to the Galactic thin and thick disks using spectra obtained with the Phoenix infrared spectrometer on the 2.1 m telescope at Kitt Peak. Abundances are determined from the (1‑0) R9 2.3358 µm feature of the molecule HF. Additionally, sodium abundances are derived in 25 …

2024 The Astronomical Journal
Gaia 0
How Solar Soft X-Ray Irradiance Is Affected by the Size of Field of View
DOI: 10.3847/1538-4357/acf9f3 Bibcode: 2024ApJ...960...91T

Takeda, Aki; Boland, Shannon

Soft X-ray images of the Sun obtained with multiple broadband filters provide a simple and useful method to calculate averaged coronal temperature and emission measure, from which we can further calculate solar X-ray irradiance in physical units, e.g., watts per square meter. However, X-ray telescopes are often designed for pursuing high spatial r…

2024 The Astrophysical Journal
Hinode 0
Extent of the Magnetotail of Venus From the Solar Orbiter, Parker Solar Probe and BepiColombo Flybys
DOI: 10.1029/2024JA032603 Bibcode: 2024JGRA..12932603E

Sorriso-Valvo, Luca; Edberg, Niklas J. T.; Persson, Moa +20 more

We analyze data from multiple flybys by the Solar Orbiter, BepiColombo, and Parker Solar Probe (PSP) missions to study the interaction between Venus' plasma environment and the solar wind forming the induced magnetosphere. Through examination of magnetic field and plasma density signatures we characterize the spatial extent and dynamics of Venus' …

2024 Journal of Geophysical Research (Space Physics)
BepiColombo SolarOrbiter VenusExpress 0
Implications of Photon-Axion Oscillations on X-Ray Observations of the Coma Cluster
DOI: 10.18524/1810-4215.2024.37.313462 Bibcode: 2024OAP....37...24S

Pulatova, N.; Tugay, A.; Zadorozhna, L. +3 more

Axion-like particles (ALPs) emerge as predictions from various extensions of the Standard Model, standing out as plausible candidates for dark matter. Axions are thought to be produced when light passes through regions of magnetic fields. This positions astrophysical environments as prime sites for their production and subsequent detection. Howeve…

2024 Odessa Astronomical Publications
XMM-Newton 0
The Sun's Magnetic Power Spectra over Two Solar Cycles. II. Cycle Dependence of Active Regions, a Magnetic Network, and Their Relation
DOI: 10.3847/1538-4357/ad5677 Bibcode: 2024ApJ...970...76L

Wang, Ruihui; Jiang, Jie; Luo, Yukun

The multiscaled solar magnetic field consists of two major components: active regions (ARs) and magnetic network. Unraveling the cycle-dependent properties and interrelations of these components is crucial for understanding the evolution of the solar magnetic field. In this study, we investigate these components using magnetic power spectra derive…

2024 The Astrophysical Journal
SOHO 0
Orbit of the Patroclus–Menoetius Binary System and Predictions for the 2024/2025 Mutual Events Season
DOI: 10.3847/1538-3881/ad1f6e Bibcode: 2024AJ....167..104B

Popescu, Marcel; Licandro, Javier; Berthier, Jérôme +5 more

We report on the ephemeris development for Menoetius, the satellite of Patroclus. Our data set consisted of ground–based and Hubble Space Telescope relative astrometry, as well as 42 lightcurves from the mutual events seasons in 2007, 2012, and 2017/2018. Our dynamical model included the effects of oblate, nonspherical shapes of the components, an…

2024 The Astronomical Journal
eHST 0
Editorial: Circulation of heavy ions and their role in regulating the near-earth plasma dynamics
DOI: 10.3389/fspas.2024.1382511 Bibcode: 2024FrASS..1182511B

Chen, Lunjin; Kronberg, Elena; Bashir, M. Fraz

2024 Frontiers in Astronomy and Space Sciences
Cluster 0
Observaciones fotométricas ópticas de candidatas a galaxias en el survey VVV
Bibcode: 2024BAAA...65..252Z

González, J. F.; Zarate, F.; Duplancic, F. +4 more

A sample of galaxy candidates observed in the south region of the galactic bulge of Vista Variables in the Via Láctea survey is presented in this work. With the use of the Double Astrograph from the Estación de Altura Carlos Ulrrico Cesco the magnitudes in the visible light of 35 galaxy candidates were obtained. This galaxy candidates were selecte…

2024 Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
Gaia 0