Search Publications

Extreme X-Ray Reflection in the Nucleus of the Seyfert Galaxy NGC 5033
DOI: 10.3847/1538-4357/ac7f30 Bibcode: 2022ApJ...935...12Y

Stern, D.; Brandt, W. N.; Fabian, A. C. +7 more

NGC 5033 is an intriguing Seyfert galaxy because its subclassification may change with time, and because optical and submillimeter observations find that the massive black hole does not sit at the dynamical center of the galaxy, pointing to a past merger. We obtained a new optical spectrum of NGC 5033 using the 200″ Hale telescope at Palomar that …

2022 The Astrophysical Journal
XMM-Newton 1
Milliarcsecond X-Ray Astrometry to Resolve Inner Regions of AGN at z > 1 Using Gravitational Lensing
DOI: 10.3847/1538-4357/ac68eb Bibcode: 2022ApJ...931...68S

Barnacka, Anna; Spingola, Cristiana; Schwartz, Daniel

We report the localization of the X-ray emission from two strongly lensed AGN, CLASS B0712+472 (z = 1.34) and CLASS B1608+656 (z = 1.394). We obtain milliarcsecond X-ray astrometry by developing a novel method that combines parametric lens modeling with a Bayesian analysis. We spatially locate the X-ray sources in CLASS B0712+472 and CLASS B1608+6…

2022 The Astrophysical Journal
eHST 1
FAST Search for Circumstellar Atomic Hydrogen. I. The Young Planetary Nebula IC 4997
DOI: 10.3847/1538-4357/ac6fdb Bibcode: 2022ApJ...933....4O

Zhang, Yong; Zhang, Chuan-Peng; Parker, Quentin A. +3 more

Using the Five-hundred-meter Aperture Spherical radio Telescope in Guizhou, China, we detect the 21 cm neutral atomic hydrogen absorption in the young planetary nebula IC 4997. The absorption arises from a shell that is also associated with Na I D lines. The H I shell has a mass of 1.46 × 10-2 M and a dynamic age of 990 yr.…

2022 The Astrophysical Journal
Gaia 1
Extreme Solar Flare-driven Short-wave Fadeout Observed by SuperDARN ZHO Radar
DOI: 10.3847/1538-4357/ac6f56 Bibcode: 2022ApJ...933...45L

Wang, M.; Liu, J.; Lu, J. Y. +6 more

Based on the observations from the Super Dual Auroral Radar Network at the Zhongshan Station (-74.9 MLAT, 97.2 MLON) and GOES satellites X-ray sensor, we present the first statistical study of the dayside ionospheric short-wave fadeout (SWF) events on the Southern Hemispheric high latitude from the years 2010-2019 and provide a normal characterist…

2022 The Astrophysical Journal
SOHO 1
Erratum: Primordial black hole origin for thermal gamma-ray bursts
DOI: 10.1093/mnras/stac681 Bibcode: 2022MNRAS.512.2925D

del Barco, Oscar

2022 Monthly Notices of the Royal Astronomical Society
INTEGRAL 1
A 2+1 + 1 quadruple star system containing the most eccentric, low-mass, short-period, eclipsing binary known
DOI: 10.1093/mnras/stab3507 Bibcode: 2022MNRAS.510.2448H

Vanderburg, A.; Zasche, P.; Borkovits, T. +12 more

We present an analysis of a newly discovered 2+1 + 1 quadruple system with TESS containing an unresolved eclipsing binary (EB) as part of TIC 121088960 and a close neighbour TIC 121088959. The EB consists of two very low-mass M dwarfs in a highly eccentric (e = 0.709) short-period (P = 3.043 58 d) orbit. Given the large pixel size of TESS and the …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 1
Spectroscopic Diagnostics of the Mid-infrared Features of the Dark Globule DC 314.8-5.1 with the Spitzer Space Telescope
DOI: 10.3847/1538-4357/ac7a42 Bibcode: 2022ApJ...934...94K

Stawarz, Ł.; Rocha, W. R. M.; Kosmaczewski, E. +2 more

We present an analysis of the mid-infrared spectra, obtained from the Spitzer Space Telescope, of the dark globule DC 314.8-5.1, which is at the onset of low-mass star formation. The target has a serendipitous association with a B-type field star that illuminates a reflection nebula in the cloud. We focus on the polycyclic aromatic hydrocarbon (PA…

2022 The Astrophysical Journal
Gaia 1
The spiral density-wave structure of the Milky Way in the 3-kpc-scale solar neighbourhood: line-of-sight velocities of 252 young open clusters
DOI: 10.1093/mnras/stac426 Bibcode: 2022MNRAS.512.1169G

Gedalin, Michael; Jiang, Ing-Guey; Griv, Evgeny

Following Lin and Shu, the spiral structure in the Milky Way disc is considered as an oscillating density-wave pattern. As such, regular enhancements in density are relatedly linked to systematic variations in velocity of young stars and stellar clusters, and interstellar gas. We explain measured line-of-sight velocities of 252 open clusters with …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 1
TIC 5724661: A Long-period Binary with a Pulsating sdB Star and δ Scuti Variable
DOI: 10.3847/1538-4357/ac84d0 Bibcode: 2022ApJ...936..123J

Rappaport, Saul A.; Jayaraman, Rahul; Bieryla, Allyson +8 more

Using TESS 20 s cadence data, we have discovered an unusual combination of pulsating stars in what we infer to be a binary system. The binary consists of a standard δ Scuti star with pulsations over the range 32-41 day-1; this is in a likely wide orbit with a hot subdwarf-B (sdB) star, which itself has a large-amplitude p-mode pulsation…

2022 The Astrophysical Journal
Gaia 1
Plasma vortices driven by magnetic torsion generated by electric currents in non-magnetic planetary wakes
DOI: 10.1016/j.asr.2022.03.002 Bibcode: 2022AdSpR..69.3902D

Flandes, Alberto; Durand-Manterola, Héctor Javier

In non-collisional magnetised astrophysical plasmas, vortices can form as it is the case of the Venus plasma wake where Lundin et al. (2013) identified a large vortex through the integration of data of many orbits from the Venus Express (VEX) spacecraft. On the one hand, our purpose is to develop a theoretical foundation in order to explain the oc…

2022 Advances in Space Research
VenusExpress 1