Search Publications

Radio Observations of Four Active Galactic Nuclei Hosting Intermediate-mass Black Hole Candidates: Studying the Outflow Activity and Evolution
DOI: 10.3847/1538-4357/ac9e9d Bibcode: 2022ApJ...941...43Y

Ho, Luis C.; Zhang, Shaohua; Yang, Jun +5 more

Observational searches for intermediate-mass black holes (IMBHs; 102-106 M ) include relatively isolated dwarf galaxies. For those that host active galactic nuclei (AGNs), the IMBH nature may be discerned through the accretion-jet activity. We present radio observations of four AGN-hosting dwarf galaxies, which po…

2022 The Astrophysical Journal
Gaia 9
Layered Ejecta Craters in the Candidate Landing Areas of China's First Mars Mission (Tianwen-1): Implications for Subsurface Volatile Concentrations
DOI: 10.1029/2021JE007089 Bibcode: 2022JGRE..12707089N

Di, Kaichang; Gou, Sheng; Yue, Zongyu +2 more

One important scientific objective of China's first Mars mission (Tianwen-1) is to investigate the martian surface soil characteristics and water-ice distribution. Layered ejecta craters (LECs) on Mars are characterized by their fluidized ejecta deposits which have been interpreted to indicate volatiles in the substrate where the impact occurred. …

2022 Journal of Geophysical Research (Planets)
MEx 9
Far-ultraviolet Flares on Accreting Protostars: Weak and Classical T Tauri Stellar Pair Analysis
DOI: 10.3847/1538-4357/ac8f26 Bibcode: 2022ApJ...939...82H

Kowalski, Adam F.; France, Kevin; Hinton, P. C. +5 more

The far-ultraviolet (FUV) emission of classical T Tauri stars (CTTSs) is known to play an important role in protoplanetary disk dispersal and giant planet formation, yet the role played by protostellar flares in these processes is largely unknown. We use nearby star-forming regions as laboratories to probe the FUV flare characteristics of CTTSs an…

2022 The Astrophysical Journal
eHST 9
First Report of a Solar Energetic Particle Event Observed by China's Tianwen-1 Mission in Transit to Mars
DOI: 10.3847/2041-8213/ac80f5 Bibcode: 2022ApJ...934L..15F

Zhao, Lingling; Sun, Zhiyu; Yu, Yuhong +15 more

Solar energetic particles (SEPs) associated with flares and/or coronal mass ejection (CME)-driven shocks can impose acute radiation hazards on space explorations. To measure energetic particles in near-Mars space, the Mars Energetic Particle Analyzer (MEPA) instrument on board China's Tianwen-1 (TW-1) mission was designed. Here, we report the firs…

2022 The Astrophysical Journal
SOHO 9
Evidence for C and Mg variations in the GD-1 stellar stream
DOI: 10.1093/mnras/stac1953 Bibcode: 2022MNRAS.515.5802B

Balbinot, Eduardo; Cabrera-Ziri, Ivan; Lardo, Carmela

Dynamically cold stellar streams are the relics left over from globular cluster dissolution. These relics offer a unique insight into a now fully disrupted population of ancient clusters in our Galaxy. Using a combination of Gaia eDR3 proper motions, optical and near-UV colours, we select a sample of likely Red Giant Branch stars from the GD-1 str…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 9
Model-independent redshift estimation of BL Lac objects through very-high-energy observations
DOI: 10.1093/mnras/stab3173 Bibcode: 2022MNRAS.511..994M

Bhatt, Nilay; Malik, Zahoor; Sahayanathan, Sunder +3 more

The very-high-energy (VHE) gamma-ray spectral indices of blazars show a strong correlation with the source redshift. The absence of any such correlation in low-energy gamma-rays and X-rays indicates the presence of extragalactic background light (EBL)-induced absorption of VHE gamma-rays. By employing a linear regression analysis, this observation…

2022 Monthly Notices of the Royal Astronomical Society
Exosat 9
Relationship between Total Solar Irradiance and Magnetic Flux during Solar Minima
DOI: 10.3847/1538-4357/ac8a98 Bibcode: 2022ApJ...936..158M

Lean, Judith L.; Marchenko, Sergey V.; DeLand, Matthew T.

What drives the small total solar irradiance (TSI) changes of ~50-100 parts per million (compared with >1000 ppm solar-cycle amplitudes) during a deep solar minimum, i.e., in the practical absence of detectable sunspots and long-lasting active regions? We consider the epoch 2008 June-October and investigate multiple data sets (TSI; various Mg I…

2022 The Astrophysical Journal
SOHO 9
A Very Long Baseline Array Trigonometric Parallax for RR Aql and the Mira Period-Luminosity Relation
DOI: 10.3847/1538-4357/ac69e0 Bibcode: 2022ApJ...931...74S

Sun, Yan; Reid, Mark J.; Zhang, Bo +4 more

We report Very Long Baseline Array observations of 22 GHz H2O and 43 GHz SiO masers toward the Mira variable RR Aql. By fitting the SiO maser emission to a circular ring, we estimate the absolute stellar position of RR Aql and find agreement with Gaia astrometry to within the joint uncertainty of ≈1 mas. Using the maser astrometry we me…

2022 The Astrophysical Journal
Gaia 9
Interplanetary Sheaths and Corotating Interaction Regions: A Comparative Statistical Study on Their Characteristics and Geoeffectiveness
DOI: 10.1007/s11207-022-02020-6 Bibcode: 2022SoPh..297...97H

Hajra, Rajkumar; Sunny, Jibin V.; Babu, Megha +1 more

Interplanetary sheaths and corotating interaction regions (CIRs), while having different solar sources, represent turbulent solar-wind plasma and magnetic field that can perturb the Earth's magnetosphere. We explore long-term solar-wind measurements upstream of the Earth during Solar Cycle 24, from January 2008 to December 2019, to compare their s…

2022 Solar Physics
SOHO 9
X-Ray Intraday Variability of the TeV Blazar Markarian 421 with XMM-Newton
DOI: 10.3847/1538-4365/ac7799 Bibcode: 2022ApJS..262....4N

Gupta, Alok C.; Gaur, Haritma; Ostrowski, Michał +4 more

Highly variable Markarian 421 is a bright high-synchrotron energy peaked blazar showing a wide featureless nonthermal spectrum, making it a good candidate for our study of intraday flux and spectral variations over time. We analyze its X-ray observations over 17 yr, taken with the EPIC-pn instrument, to probe into the intraday variability properti…

2022 The Astrophysical Journal Supplement Series
XMM-Newton 9