Search Publications

Evidence for a Rotational Component in the Circumgalactic Medium of Nearby Galaxies
DOI: 10.3847/1538-4357/ab9905 Bibcode: 2020ApJ...897..151F

Wakker, Bart P.; French, David M.

We present results of a study comparing the relative velocity of Lyα absorbers to the rotation velocity of nearby galaxy disks in the local universe (z ≤ 0.03). We have obtained rotation curves via long-slit spectroscopy of eight galaxies with the Southern African Large Telescope, and combine this data set with an additional 16 galaxies with data …

2020 The Astrophysical Journal
eHST 14
Chemically Peculiar A and F Stars with Enhanced s-process and Iron-peak Elements: Stellar Radiative Acceleration at Work
DOI: 10.3847/1538-4357/ab99a5 Bibcode: 2020ApJ...898...28X

Ting, Yuan-Sen; Rix, Hans-Walter; Zhang, Meng +6 more

We present ≳15,000 metal-rich ([Fe/H] > -0.2 dex) A and F stars whose surface abundances deviate strongly from solar abundance ratios and cannot plausibly reflect their birth material composition. These stars are identified by their high [Ba/Fe] abundance ratios ([Ba/Fe] > 1.0 dex) in the LAMOST DR5 spectra analyzed by Xiang et al. They are …

2020 The Astrophysical Journal
Gaia 14
Chandra Monitoring of the J1809-1917 Pulsar Wind Nebula and Its Field
DOI: 10.3847/1538-4357/abaf4b Bibcode: 2020ApJ...901..157K

Pavlov, George G.; Kargaltsev, Oleg; Klingler, Noel +3 more

PSR J1809-1917 is a young (τ = 51 kyr) and energetic ( $\dot{E}=1.8\times {10}^{36}$ erg s-1) radio pulsar powering an X-ray pulsar wind nebula (PWN) that exhibits morphological variability. We report on the results of a new monitoring campaign by the Chandra X-ray Observatory (Chandra), carried out across six epochs with a ∼7 week cade…

2020 The Astrophysical Journal
Gaia XMM-Newton 14
A Rapidly Varying Red Supergiant X-Ray Binary in the Galactic Center
DOI: 10.3847/1538-4357/ab90ff Bibcode: 2020ApJ...896...32G

Gottlieb, Amy M.; Ackley, Kendall; DeWitt, Curtis +2 more

We analyzed multiwavelength observations of the previously identified Galactic center X-ray binary CXO 174528.79-290942.8 (XID 6592) and determine that the near-infrared counterpart is a red supergiant based on its spectrum and luminosity. Scutum X-1 is the only previously known X-ray binary with a red supergiant donor star and closely resembles X…

2020 The Astrophysical Journal
XMM-Newton 14
The Detection of Dust Gap-ring Structure in the Outer Region of the CR Cha Protoplanetary Disk
DOI: 10.3847/1538-4357/ab5d2b Bibcode: 2020ApJ...888...72K

Dong, Ruobing; Kataoka, Akimasa; Sitko, Michael +13 more

We observe the dust continuum at 225 GHz and CO isotopologue (12CO, 13CO, and C18O) J = 2-1 emission lines toward the CR Cha protoplanetary disk using the Atacama Large Millimeter/submillimeter Array. The dust continuum image shows a dust gap-ring structure in the outer region of the dust disk. A faint dust ring is…

2020 The Astrophysical Journal
Gaia 14
A Model-insensitive Baryon Acoustic Oscillation Feature in the 21 cm Signal from Reionization
DOI: 10.3847/1538-4357/aba26a Bibcode: 2020ApJ...898..168C

Trac, Hy; Cain, Christopher; D'Aloisio, Anson +2 more

We examine the impact of baryon-dark matter relative velocities on intergalactic small-scale structure and the 21 cm signal during reionization. Streaming velocities reduced clumping in the intergalactic medium on mass scales of ∼104-108 M. This effect produced a distinct baryon acoustic oscillation (BAO) feature …

2020 The Astrophysical Journal
eHST 14
Magnetohydrodynamic Turbulent Evolution of a Magnetic Cloud in the Outer Heliosphere
DOI: 10.3847/2041-8213/abcb03 Bibcode: 2020ApJ...905L..12T

Telloni, Daniele; Zank, Gary P.; Adhikari, Laxman +8 more

This Letter exploits joint observations of the same interplanetary coronal mass ejection by widely separated spacecraft to study, for the first time, the turbulent evolution of the magnetohydrodynamic (MHD) properties of the embedded magnetic cloud, during its propagation throughout interplanetary space. Specifically, the event was observed by Win…

2020 The Astrophysical Journal
Ulysses 14
On the Correlation between L Dwarf Optical and Infrared Variability and Radio Aurorae
DOI: 10.3847/1538-4357/abb826 Bibcode: 2020ApJ...903...74R

Richey-Yowell, Tyler; Kao, Melodie M.; Pineda, J. Sebastian +2 more

Photometric variability attributed to cloud phenomena is common in L/T transition brown dwarfs. Recent studies show that such variability may also trace aurorae, suggesting that localized magnetic heating may contribute to observed brown dwarf photometric variability. We assess this potential correlation with a survey of 17 photometrically variabl…

2020 The Astrophysical Journal
Gaia 14
Observation and Modeling of High-temperature Solar Active Region Emission during the High-resolution Coronal Imager Flight of 2018 May 29
DOI: 10.3847/1538-4357/ab917c Bibcode: 2020ApJ...896...51W

Golub, Leon; Winebarger, Amy R.; Warren, Harry P. +15 more

Excellent coordinated observations of NOAA active region 12712 were obtained during the flight of the High-resolution Coronal Imager (Hi-C) sounding rocket on 2018 May 29. This region displayed a typical active region core structure with relatively short, high-temperature loops crossing the polarity inversion line and bright "moss" located at the …

2020 The Astrophysical Journal
Hinode IRIS 14
Evidence of Particle Acceleration in the Superbubble 30 Doradus C with NuSTAR
DOI: 10.3847/1538-4357/ab8232 Bibcode: 2020ApJ...893..144L

Auchettl, Katie; Madsen, Kristin K.; Grefenstette, Brian W. +2 more

We present evidence of diffuse, non-thermal X-ray emission from the superbubble 30 Doradus C (30 Dor C) using hard X-ray images and spectra from NuSTAR observations. For this analysis, we utilize data from a 200 ks targeted observation of 30 Dor C as well as 2.8 Ms of serendipitous off-axis observations from the monitoring of nearby SN 1987A. The …

2020 The Astrophysical Journal
XMM-Newton 14