Search Publications

The Synchrotron Emission Pattern of Intrabinary Shocks
DOI: 10.3847/1538-4357/ab24d9 Bibcode: 2019ApJ...879...73K

An, Hongjun; Romani, Roger W.; Kandel, D.

We model millisecond pulsar winds colliding with radiatively driven companion winds in black widow and redback systems. For the redbacks, the geometry of this intrabinary shock (IBS) is quite sensitive to the expected equatorial concentration in the pulsar outflow. We thus analytically extend IBS thin-shock models to ∼ {\sin }2nθ pulsar…

2019 The Astrophysical Journal
XMM-Newton 35
CHEERS Results from NGC 3393. III. Chandra X-Ray Spectroscopy of the Narrow Line Region
DOI: 10.3847/1538-4357/aaf4f5 Bibcode: 2019ApJ...872...94M

Elvis, Martin; Raymond, John; Risaliti, Guido +6 more

We present spatially resolved Chandra narrow-band imaging and imaging spectroscopy of NGC 3393. This galaxy hosts a Compton-thick Seyfert 2 active galactic nucleus (AGN) with sub-kpc bipolar outflows that are strongly interacting with the circumnuclear gas. We identify narrow-band excess emission associated with the Ne IX 0.905 keV transition (wit…

2019 The Astrophysical Journal
eHST 35
Exploring the Outskirts of Globular Clusters: The Peculiar Kinematics of NGC 3201
DOI: 10.3847/2041-8213/ab58d1 Bibcode: 2019ApJ...887L..12B

Famaey, B.; Ibata, R.; Bianchini, P.

The outskirts of globular clusters (GCs) simultaneously retain crucial information about their formation mechanism and the properties of their host galaxy. Thanks to the advent of precision astrometry both their morphological and kinematic properties are now accessible. Here we present the first dynamical study of the outskirts of the retrograde G…

2019 The Astrophysical Journal
Gaia 35
Late-time Kilonova Light Curves and Implications to GW170817
DOI: 10.3847/1538-4357/ab1f71 Bibcode: 2019ApJ...878...93W

Waxman, Eli; Ofek, Eran O.; Kushnir, Doron

We discuss the late-time (tens of days) emission from the radioactive ejecta of mergers involving neutron stars, when the ionization energy loss time of beta-decay electrons and positrons exceeds the expansion time. We show that if the e± are confined to the plasma (by magnetic fields), then the time dependence of the plasma heating rat…

2019 The Astrophysical Journal
eHST 35
The Role of Major Mergers and Nuclear Star Formation in Nearby Obscured Quasars
DOI: 10.3847/1538-4357/ab1921 Bibcode: 2019ApJ...877...52Z

Ho, Luis C.; Zhao, Dongyao; Kim, Minjin +2 more

We investigate the triggering mechanism and the structural properties of obscured luminous active galactic nuclei from a detailed study of the rest-frame B and I Hubble Space Telescope images of 29 nearby (z ≈ 0.04-0.4) optically selected type 2 quasars. Morphological classification reveals that only a minority (34%) of the hosts are mergers or in…

2019 The Astrophysical Journal
eHST 35
Tidal Destruction in a Low-mass Galaxy Environment: The Discovery of Tidal Tails around DDO 44
DOI: 10.3847/1538-4357/ab4c32 Bibcode: 2019ApJ...886..109C

Forbes, Duncan A.; Romanowsky, Aaron J.; Strader, Jay +10 more

We report the discovery of a ≳1° (∼50 kpc) long stellar tidal stream emanating from the dwarf galaxy DDO 44, a likely satellite of Local Volume galaxy NGC 2403 located ∼70 kpc in projection from its companion. NGC 2403 is a roughly Large Magellanic Cloud (LMC) stellar-mass galaxy 3 Mpc away, residing at the outer limits of the M81 group. We are ma…

2019 The Astrophysical Journal
eHST 35
Direct Estimates of the Solar Coronal Magnetic Field Using Contemporaneous Extreme-ultraviolet, Radio, and White-light Observations
DOI: 10.3847/1538-4357/ab2adf Bibcode: 2019ApJ...881...24K

Kumari, Anshu; Ramesh, R.; Kathiravan, C. +2 more

We report a solar coronal split-band type II radio burst that was observed on 2016 March 16 with the Gauribidanur Radio Spectro-Polarimeter in the frequency range ≈90-50 MHz, and the Gauribidanur RadioheliograPH at two discrete frequencies, viz. 80 and 53.3 MHz. Observations around the same epoch in extreme ultraviolet (EUV) and white light show t…

2019 The Astrophysical Journal
SOHO 35
Transient Inverse-FIP Plasma Composition Evolution within a Solar Flare
DOI: 10.3847/1538-4357/ab07c1 Bibcode: 2019ApJ...875...35B

Long, David M.; Matthews, Sarah A.; Brooks, David H. +9 more

Understanding elemental abundance variations in the solar corona provides an insight into how matter and energy flow from the chromosphere into the heliosphere. Observed variations depend on the first ionization potential (FIP) of the main elements of the Sun’s atmosphere. High-FIP elements (>10 eV) maintain photospheric abundances in the coron…

2019 The Astrophysical Journal
Hinode 34
On a New Method to Estimate the Distance, Reddening, and Metallicity of RR Lyrae Stars Using Optical/Near-infrared (B, V, I, J, H, K) Mean Magnitudes: ω Centauri as a First Test Case
DOI: 10.3847/1538-4357/aaf23f Bibcode: 2019ApJ...870..115B

Walker, A. R.; Mateo, M.; Valenti, E. +26 more

We developed a new approach to provide accurate estimates of the metal content, reddening, and true distance modulus of RR Lyrae stars (RRLs). The method is based on homogeneous optical (BVI) and near-infrared (JHK) mean magnitudes and on predicted period-luminosity-metallicity relations (IJHK) and absolute mean magnitude-metallicity relations (BV…

2019 The Astrophysical Journal
Gaia 34
Anchor Point of Electron Acceleration around Dipolarization Fronts in Space Plasmas
DOI: 10.3847/2041-8213/ab06cb Bibcode: 2019ApJ...873L...2L

Fu, H. S.; Liu, C. M.

An anchor point, which is an energy threshold above which electrons are accelerated and below which electrons are decelerated, has recently been reported within the dipolarizing flux bundles behind dipolarization fronts (DFs) both in observations and simulations. However, what determines this point and how it is formed remain unclear. In this stud…

2019 The Astrophysical Journal
Cluster 34