Search Publications

Hubble Space Telescope Imaging of Antlia B: Star Formation History and a New Tip of the Red Giant Branch Distance
DOI: 10.3847/1538-4357/ab58d2 Bibcode: 2020ApJ...888...31H

Carlin, J. L.; Dolphin, A. E.; Crnojević, D. +8 more

A census of the satellite population around dwarf galaxy primary hosts in environments outside the Local Group is essential to understanding Λ cold dark matter galaxy formation and evolution on the smallest scales. We present deep optical Hubble Space Telescope imaging of the gas-rich, faint dwarf galaxy Antlia B (M V = -9.4)—a likely…

2020 The Astrophysical Journal
eHST 18
Coronal Mini-jets in an Activated Solar Tornado-like Prominence
DOI: 10.3847/1538-4357/ab9cad Bibcode: 2020ApJ...899...19C

Zhang, Jun; De Pontieu, Bart; Kliem, Bernhard +3 more

High-resolution observations from the Interface Region Imaging Spectrometer reveal the existence of a particular type of small solar jet, which arose singly or in clusters from a tornado-like prominence suspended in the corona. In this study, we perform a detailed statistical analysis of 43 selected mini-jets in the tornado event. Our results show…

2020 The Astrophysical Journal
IRIS 18
Dynamical Masses of Young Stars. II. Young Taurus Binaries Hubble 4, FF Tau, and HP Tau/G3
DOI: 10.3847/1538-4357/ab5aed Bibcode: 2020ApJ...889..175R

Rizzuto, Aaron C.; Dupuy, Trent J.; Ireland, Michael J. +1 more

One of the most effective ways to test stellar evolutionary models is to measure dynamical masses for binary systems at a range of temperatures. In this paper, we present orbits of three young K+M binary systems in Taurus (Hubble 4, FF Tau, and HP Tau/G3) with very long baseline interferometry parallaxes. We obtained precision astrometry with Keck…

2020 The Astrophysical Journal
Gaia eHST 18
Turbulence and Energetic Particles in Radiative Shock Waves in the Cygnus Loop. II. Development of Postshock Turbulence
DOI: 10.3847/1538-4357/abb821 Bibcode: 2020ApJ...903....2R

Blair, William P.; Slavin, Jonathan D.; Raymond, John C. +3 more

Radiative shock waves in the Cygnus Loop and other supernova remnants show different morphologies in [O III] and Hα emission. We use HST spectra and narrowband images to study the development of turbulence in the cooling region behind a shock on the west limb of the Cygnus Loop. We refine our earlier estimates of shock parameters that were based u…

2020 The Astrophysical Journal
eHST 18
Numerical Modeling of Suprathermal Electron Transport in the Solar Wind: Effects of Whistler Turbulence
DOI: 10.3847/1538-4357/ab7a93 Bibcode: 2020ApJ...892...95T

Zank, Gary P.; Tang, Bofeng; Kolobov, Vladimir I.

The solar wind electron velocity distribution function deviates significantly from an equilibrium Maxwellian distribution and is composed of a Maxwellian core, a suprathermal halo, a field-aligned component strahl, and a higher-energy superhalo. Wave-particle interactions associated with whistler wave turbulence are introduced into the kinetic tra…

2020 The Astrophysical Journal
Cluster Ulysses 18
Significant Suppression of Star Formation in Radio-quiet AGN Host Galaxies with Kiloparsec-scale Radio Structures
DOI: 10.3847/1538-4357/abc3c4 Bibcode: 2020ApJ...904...83S

Koss, Michael; Ricci, Claudio; Mushotzky, Richard +4 more

We conducted 22 GHz 1″ Jansky Very Large Array imaging of 100 radio-quiet X-ray-selected active galactic nuclei (AGN) from the Swift-Burst Array Telescope (Swift-BAT) survey. We find AGN-driven kiloparsec-scale radio structures inconsistent with pure star formation in 11 AGN. The host galaxies of these AGN lie significantly below the star-forming …

2020 The Astrophysical Journal
Herschel eHST 18
Modeling the Precession of the Warped Inner Accretion Disk in the Pulsars LMC X-4 and SMC X-1 with NuSTAR and XMM-Newton
DOI: 10.3847/1538-4357/ab5b04 Bibcode: 2020ApJ...888..125B

Pottschmidt, Katja; Wilms, Jörn; Hickox, Ryan C. +3 more

We present a broadband X-ray study of the effect of superorbital periods on X-ray spectra and pulse profiles in the neutron star X-ray binaries LMC X-4 and SMC X-1. These two sources display periodic or quasiperiodic variations in luminosity of the order of tens of days, which are known to be superorbital, and are attributed to warped, precessing …

2020 The Astrophysical Journal
XMM-Newton 18
The Strikingly Metal-rich Halo of the Sombrero Galaxy
DOI: 10.3847/1538-4357/ab64e9 Bibcode: 2020ApJ...890...52C

Cohen, Roger E.; Chandar, Rupali; Goudfrooij, Paul +5 more

The nature of the Sombrero galaxy (M104 = NGC 4594) has remained elusive despite many observational studies at a variety of wavelengths. Here we present Hubble Space Telescope imaging of two fields at ∼16 and 33 kpc along the minor axis to examine stellar metallicity gradients in the extended spheroid. We use this imaging, extending more than 2 ma…

2020 The Astrophysical Journal
eHST 18
A DESGW Search for the Electromagnetic Counterpart to the LIGO/Virgo Gravitational-wave Binary Neutron Star Merger Candidate S190510g
DOI: 10.3847/1538-4357/abb823 Bibcode: 2020ApJ...903...75G

Smith, M.; Lidman, C.; Rest, A. +90 more

We present the results from a search for the electromagnetic counterpart of the LIGO/Virgo event S190510g using the Dark Energy Camera (DECam). S190510g is a binary neutron star (BNS) merger candidate of moderate significance detected at a distance of 227 ± 92 Mpc and localized within an area of 31 (1166) square degrees at 50% (90%) confidence. Wh…

2020 The Astrophysical Journal
Gaia 18
Near-infrared Spectroscopy of CK Vulpeculae: Revealing a Remarkably Powerful Blast from the Past
DOI: 10.3847/2041-8213/abc885 Bibcode: 2020ApJ...904L..23B

Gehrz, R. D.; Shahbandeh, M.; Eyres, S. P. S. +6 more

CK Vulpeculae (CK Vul), which erupted in AD 1670-71, was long considered to be a nova outburst; however, recent observations have required that alternative scenarios be considered. Long-slit infrared spectroscopy of a forbidden line of iron reported here has revealed high line-of-sight velocities (∼±900 km s-1) of the ansae at the tips …

2020 The Astrophysical Journal
Gaia 17