Search Publications

NICER X-Ray Observations of Seven Nearby Rotation-powered Millisecond Pulsars
DOI: 10.3847/2041-8213/ab511b Bibcode: 2019ApJ...887L..27G

Chakrabarty, Deepto; Bogdanov, Slavko; Deneva, Julia S. +18 more

The Neutron star Interior Composition Explorer observed several rotation-powered millisecond pulsars (MSPs) to search for or confirm the presence of X-ray pulsations. When broad and sine-like, these pulsations may indicate thermal emission from hot polar caps at the magnetic poles on the neutron star surface. We report confident detections (≥4.7σ …

2019 The Astrophysical Journal
Gaia XMM-Newton 61
Multi-wavelength Properties of Type 1 and Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey
DOI: 10.3847/1538-4357/ab01fb Bibcode: 2019ApJ...872..168S

Lusso, Elisabeta; Marchesi, Stefano; Onodera, Masato +6 more

We investigate the multi-wavelength properties of host galaxies of 3701 X-ray-selected active galactic nuclei (AGNs) out to z ∼ 5 in the Chandra-COSMOS Legacy Survey. Thanks to the extensive multi-wavelength photometry available in the COSMOS field, we derive AGN luminosities, host stellar masses, and star formation rates (SFRs) via a multi-compon…

2019 The Astrophysical Journal
Herschel 61
Dissecting the AGN Disk-Jet System with Joint VLBI-Gaia Analysis
DOI: 10.3847/1538-4357/aaf650 Bibcode: 2019ApJ...871..143P

Kovalev, Y. Y.; Plavin, A. V.; Petrov, L. Y.

We analyze differences in positions of active galactic nuclei (AGNs) between Gaia data release 2 and very long baseline interferometry (VLBI) and compare the significant VLBI-to-Gaia offsets in more than 1000 objects with their jet directions. Remarkably at least three-fourths of the significant offsets are confirmed to occur downstream or upstrea…

2019 The Astrophysical Journal
Gaia 61
Ambient Column Densities of Highly Ionized Oxygen in Precipitation-limited Circumgalactic Media
DOI: 10.3847/1538-4357/ab2bfd Bibcode: 2019ApJ...880..139V

Voit, G. Mark

Many of the baryons associated with a galaxy reside in its circumgalactic medium (CGM), in a diffuse volume-filling phase at roughly the virial temperature. Much of the oxygen produced over cosmic time by the galaxy’s stars also ends up there. The resulting absorption lines in the spectra of UV and X-ray background sources are powerful diagnostics…

2019 The Astrophysical Journal
eHST 59
Evidence for an Aspherical Population III Supernova Explosion Inferred from the Hyper-metal-poor Star HE 1327-2326
DOI: 10.3847/1538-4357/ab14e7 Bibcode: 2019ApJ...876...97E

Placco, Vinicius M.; Tominaga, Nozomu; Nomoto, Ken'ichi +6 more

We present observational evidence that an aspherical supernova explosion could have occurred in the first stars in the early universe. Our results are based on the first determination of a Zn abundance in a Hubble Space Telescope/Cosmic Origins Spectrograph high-resolution UV spectrum of a hyper-metal-poor (HMP) star, HE 1327-2326, with {{[Fe/H]}}…

2019 The Astrophysical Journal
Gaia eHST 59
SI IV Resonance Line Emission during Solar Flares: Non-LTE, Nonequilibrium, Radiation Transfer Simulations
DOI: 10.3847/1538-4357/aaf46e Bibcode: 2019ApJ...871...23K

Kerr, Graham S.; Carlsson, Mats; Young, Peter R. +2 more

The Interface Region Imaging Spectrograph routinely observes the Si IV resonance lines. When analyzing quiescent observations of these lines, it has typically been assumed that they form under optically thin conditions. This is likely valid for the quiescent Sun, but this assumption has also been applied to the more extreme flaring scenario. We us…

2019 The Astrophysical Journal
IRIS 59
The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-mass Selected Galaxies Using MUSE Spectroscopy
DOI: 10.3847/1538-4357/ab3102 Bibcode: 2019ApJ...882..140B

Carilli, Chris; Somerville, Rachel S.; Bacon, Roland +31 more

We discuss the nature and physical properties of gas-mass selected galaxies in the ALMA spectroscopic survey (ASPECS) of the Hubble Ultra Deep Field (HUDF). We capitalize on the deep optical integral-field spectroscopy from the Multi Unit Spectroscopic Explorer (MUSE) HUDF Survey and multiwavelength data to uniquely associate all 16 line emitters,…

2019 The Astrophysical Journal
eHST 58
Validation of the Alfvén Wave Solar Atmosphere Model (AWSoM) with Observations from the Low Corona to 1 au
DOI: 10.3847/1538-4357/ab4f5e Bibcode: 2019ApJ...887...83S

van der Holst, Bart; Lamy, Philippe; Vásquez, Alberto M. +9 more

We perform a validation study of the latest version of the Alfvén Wave Solar atmosphere Model (AWSoM) within the Space Weather Modeling Framework. To do so, we compare the simulation results of the model with a comprehensive suite of observations for Carrington rotations representative of the solar minimum conditions extending from the solar coron…

2019 The Astrophysical Journal
SOHO Ulysses 58
Global 3D Hydrodynamic Modeling of In-transit Lyα Absorption of GJ 436b
DOI: 10.3847/1538-4357/ab46a4 Bibcode: 2019ApJ...885...67K

Lammer, H.; Khodachenko, M. L.; Shaikhislamov, I. F. +5 more

Using a global 3D, fully self-consistent, multifluid hydrodynamic model, we simulate the escaping upper atmosphere of the warm Neptune GJ 436b, driven by the stellar X-ray and ultraviolet (XUV) radiation impact and gravitational forces and interacting with the stellar wind. Under the typical parameters of XUV flux and stellar wind plasma expected …

2019 The Astrophysical Journal
eHST 58
Morphologies of ∼190,000 Galaxies at z = 0-10 Revealed with HST Legacy Data. III. Continuum Profile and Size Evolution of Lyα Emitters
DOI: 10.3847/1538-4357/aaf64b Bibcode: 2019ApJ...871..164S

Ouchi, Masami; Harikane, Yuichi; Shibuya, Takatoshi +1 more

We present the redshift evolution of the radial surface brightness profile of the rest-frame UV and optical stellar continua for 9119 Lyα emitters (LAEs) at z ≃ 0-8 and 0-2, respectively. Using Hubble Space Telescope data and the LAE catalogs taken from the literature, we derive the structural quantities of the 9119 LAEs, and of ≃180,000 of photo-…

2019 The Astrophysical Journal
eHST 58