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
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
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
Solar Orbiter Observations of Proton and Alpha Particle Kinetic Signatures Related to the Presence of Switchbacks in the Inner Heliosphere: A Case Study
DOI: 10.3847/1538-4357/ad65db Bibcode: 2024ApJ...973..171P

Telloni, Daniele; D'Amicis, Raffaella; Perrone, Denise +6 more

We investigate how ions, namely protons and alpha particles, kinetically react to the presence of strong deflections in the magnetic field, the so-called switchbacks, in the first stream of slow Alfvénic wind observed by Solar Orbiter at the heliocentric distance of 0.64 au. We focus on an isolated, large-scale switchback, and we study in detail i…

2024 The Astrophysical Journal
SolarOrbiter 0
Source Region and Launch Characteristics of Magnetic-arch-blowout Solar Coronal Mass Ejections Driven by Homologous Compact-flare Blowout Jets
DOI: 10.3847/1538-4357/ad4995 Bibcode: 2024ApJ...969...48P

Joshi, Bhuwan; Moore, Ronald L.; Sterling, Alphonse C. +1 more

We study the formation of four coronal mass ejections (CMEs) originating from homologous blowout jets. All of the blowout jets originated from NOAA Active Region (AR) 11515 on 2012 July 2, within a time interval of ≈14 hr. All of the CMEs were wide (angular widths ≈ 95°–150°), and propagated with speeds ranging between ≈300 and 500 km s‑1

2024 The Astrophysical Journal
Hinode SOHO 0
Statistics of Solar White-light Flares. I. Optimization and Application of Identification Methods
DOI: 10.3847/1538-4357/ad793b Bibcode: 2024ApJ...975...69C

Hou, Yijun; Li, Ting; Liu, Jifeng +1 more

White-light flares (WLFs) are energetic activity in the stellar atmosphere. However, observed solar WLFs are relatively rare compared to stellar WLFs or solar flares observed at other wavelengths, which limits our further understanding of solar/stellar WLFs through statistical studies. By analyzing flare observations from the Solar Dynamics Observ…

2024 The Astrophysical Journal
SOHO 0
XMM-Newton Perspective of the Unique Magnetic Binary-ϵ Lupi
DOI: 10.3847/1538-4357/ad7028 Bibcode: 2024ApJ...974..182B

Wade, Gregg A.; Biswas, Ayan; Chandra, Poonam +3 more

The ϵ Lupi A (HD 136504) system stands out among magnetic massive binaries as the only short-period binary system in which both components have detectable magnetic fields. The proximity of the magnetospheres of the components leads to magnetospheric interactions, which are revealed as periodic pulses in the radio light curve of this system. In thi…

2024 The Astrophysical Journal
XMM-Newton 0
Transition Region Brightening in a Moss Region and Their Relation with Lower Atmospheric Dynamics
DOI: 10.3847/1538-4357/ad84e1 Bibcode: 2024ApJ...977...25R

Joshi, Jayant; Chen, Yajie; Yurchyshyn, Vasyl +5 more

Small-scale brightenings (SBs) are commonly observed in the transition region (TR) that separates the solar chromosphere from the corona. These brightenings, omnipresent in active region patches known as "moss" regions, could potentially contribute to the heating of active region plasma. In this study, we investigate the properties of SB events in…

2024 The Astrophysical Journal
IRIS 0
KIC 8840638: A Newly Discovered Eclipsing Binary with δ Scuti–Type Oscillations
DOI: 10.3847/1538-4357/ad7841 Bibcode: 2024ApJ...975..171Y

Yang, Tao-Zhi; Zuo, Zhao-Yu; Liu, Jun-Hui +4 more

In this paper, we analyze the light variation of KIC 8840638 using high-precision time-series data from the Kepler mission. The analysis reveals that this target is a new detached eclipsing binary system with a δ Scuti component, rather than a single δ Scuti star as previously known. The frequency analysis of short-cadence data reveals 95 signific…

2024 The Astrophysical Journal
Gaia 0