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Compton-thick AGN in the NuSTAR Era. VIII. A joint NuSTAR-XMM-Newton Monitoring of the Changing-look Compton-thick AGN NGC 1358
DOI: 10.3847/1538-4357/ac80be Bibcode: 2022ApJ...935..114M

Pozzi, F.; Buchner, J.; Feltre, A. +18 more

We present the multi-epoch monitoring with NuSTAR and XMM-Newton of NGC 1358, a nearby Seyfert 2 galaxy whose properties made it a promising candidate X-ray changing-look active galactic nucleus (AGN), i.e., a source whose column density could transition from its 2017 Compton-thick (having LOS hydrogen column density N H,LOS > 10

2022 The Astrophysical Journal
XMM-Newton 21
Extragalactic Magnetism with SOFIA (SALSA Legacy Program). III. First Data Release and On-the-fly Polarization Mapping Characterization
DOI: 10.3847/1538-4357/ac83ac Bibcode: 2022ApJ...936...65L

Beckman, John E.; Reach, William T.; Dale, Daniel A. +17 more

We describe the data processing of the Survey on extragALactic magnetiSm with SOFIA (SALSA Legacy Program). This first data release presents 33% (51.34 hr out of 155.7 hr, including overheads) of the total awarded time from 2020 January to 2021 December. Our observations were performed using the newly implemented on-the-fly mapping (OTFMAP) techni…

2022 The Astrophysical Journal
Herschel 21
Additional Evidence for a Pulsar Wind Nebula in the Heart of SN 1987A from Multiepoch X-Ray Data and MHD Modeling
DOI: 10.3847/1538-4357/ac679d Bibcode: 2022ApJ...931..132G

Greco, Emanuele; Vink, Jacco; Miceli, Marco +9 more

Since the day of its explosion, supernova (SN) 1987A has been closely monitored to study its evolution and to detect its central compact relic. In fact, the formation of a neutron star is strongly supported by the detection of neutrinos from the SN. However, besides the detection in the Atacama Large Millimeter/submillimeter Array (ALMA) data of a…

2022 The Astrophysical Journal
XMM-Newton 21
A Coronal Mass Ejection and Magnetic Ejecta Observed In Situ by STEREO-A and Wind at 55° Angular Separation
DOI: 10.3847/1538-4357/ac602f Bibcode: 2022ApJ...929..149L

Lugaz, Noé; Zhuang, Bin; Scolini, Camilla +8 more

We present an analysis of in situ and remote-sensing measurements of a coronal mass ejection (CME) that erupted on 2021 February 20 and impacted both the Solar TErrestrial RElations Observatory (STEREO)-A and the Wind spacecraft, which were separated longitudinally by 55°. Measurements on 2021 February 24 at both spacecraft are consistent with the…

2022 The Astrophysical Journal
SOHO 21
Toward Improved Understanding of Magnetic Fields Participating in Solar Flares: Statistical Analysis of Magnetic Fields within Flare Ribbons
DOI: 10.3847/1538-4357/ac3af3 Bibcode: 2022ApJ...926...56K

Savcheva, Antonia; Kazachenko, Maria D.; Lynch, Benjamin J. +2 more

Violent solar flares and coronal mass ejections (CMEs) are magnetic phenomena. However, how magnetic fields reconnecting in the flare differ from nonflaring magnetic fields remains unclear owing to the lack of studies of the flare magnetic properties. Here we present a first statistical study of flaring (highlighted by flare ribbons) vector magnet…

2022 The Astrophysical Journal
SOHO 21
Solar Flare Heating with Turbulent Suppression of Thermal Conduction
DOI: 10.3847/1538-4357/ac69e8 Bibcode: 2022ApJ...931...60A

Gordon Emslie, A.; Kerr, Graham S.; Allred, Joel C.

During solar flares, plasma is typically heated to very high temperatures, and the resulting redistribution of energy via thermal conduction is a primary mechanism transporting energy throughout the flaring solar atmosphere. The thermal flux is usually modeled using Spitzer's theory, which is based on local Coulomb collisions between the electrons…

2022 The Astrophysical Journal
Hinode 21
Expanding Bipolar X-Ray Structure After the 2006 Eruption of RS Oph
DOI: 10.3847/1538-4357/ac4583 Bibcode: 2022ApJ...926..100M

Mukai, K.; Sokoloski, J. L.; Luna, G. J. M. +2 more

We report on the detection and analysis of extended X-ray emission by the Chandra X-ray Observatory stemming from the 2006 eruption of the recurrent nova RS Oph. The extended emission was detected 1254 and 1927 days after the start of the 2006 eruption and is consistent with a bipolar flow oriented in the East-West direction of the sky with openin…

2022 The Astrophysical Journal
Gaia 21
Quasars with Proper Motions and the Link to Double and Multiple AGNs
DOI: 10.3847/1538-4357/ac7047 Bibcode: 2022ApJ...933...28M

Secrest, Nathan J.; Makarov, Valeri V.

Gaia used a large sample of photometrically selected active galactic nuclei (AGNs) and quasars to remove the residual spin of its global proper motion system in order to achieve a maximally inertial reference frame. A small fraction of these reference objects have statistically significant astrometric proper motions in Gaia EDR3. We compile a sour…

2022 The Astrophysical Journal
Gaia 21
Mixing Interstellar Clouds Surrounding the Sun
DOI: 10.3847/2041-8213/ac9120 Bibcode: 2022ApJ...937L..32S

Zank, Gary P.; Redfield, Seth; Winslow, Réka M. +9 more

On its journey through the Galaxy, the Sun passes through diverse regions of the interstellar medium. High-resolution spectroscopic measurements of interstellar absorption lines in spectra of nearby stars show absorption components from more than a dozen warm partially ionized clouds within 15 pc of the Sun. The two nearest clouds-the Local Inters…

2022 The Astrophysical Journal
Ulysses 21
Kepler-167e as a Probe of the Formation Histories of Cold Giants with Inner Super-Earths
DOI: 10.3847/1538-4357/ac3ed6 Bibcode: 2022ApJ...926...62C

Knutson, Heather A.; Fulton, Benjamin J.; Howard, Andrew W. +6 more

The observed correlation between outer giant planets and inner super-Earths is emerging as an important constraint on planet formation theories. In this study, we focus on Kepler-167, which is currently the only system known to contain both inner transiting super-Earths and a confirmed outer transiting gas giant companion beyond 1 au. Using long-t…

2022 The Astrophysical Journal
Gaia 21