Search Publications

A Population of Bona Fide Intermediate-mass Black Holes Identified as Low-luminosity Active Galactic Nuclei
DOI: 10.3847/1538-4357/aad184 Bibcode: 2018ApJ...863....1C

Boutsia, Konstantina; Chilingarian, Igor V.; Zolotukhin, Ivan Yu. +4 more

Nearly every massive galaxy harbors a supermassive black hole (SMBH) in its nucleus. SMBH masses are millions to billions of solar mass, and they correlate with properties of spheroids of their host galaxies. While the SMBH growth channels, mergers, and gas accretion are well established, their origin remains uncertain: they could have emerged eit…

2018 The Astrophysical Journal
XMM-Newton eHST 168
The Chemical Homogeneity of Sun-like Stars in the Solar Neighborhood
DOI: 10.3847/1538-4357/aad908 Bibcode: 2018ApJ...865...68B

Dreizler, Stefan; Bedell, Megan; Casagrande, Luca +9 more

The compositions of stars are a critical diagnostic tool for many topics in astronomy such as the evolution of our Galaxy, the formation of planets, and the uniqueness of the Sun. Previous spectroscopic measurements indicate a large intrinsic variation in the elemental abundance patterns of stars with similar overall metal content. However, system…

2018 The Astrophysical Journal
Gaia 163
CO and Dust Properties in the TW Hya Disk from High-resolution ALMA Observations
DOI: 10.3847/1538-4357/aaa1e7 Bibcode: 2018ApJ...852..122H

Hughes, A. Meredith; Wilner, David J.; Cleeves, L. Ilsedore +10 more

We analyze high angular resolution ALMA observations of the TW Hya disk to place constraints on the CO and dust properties. We present new, sensitive observations of the 12CO J = 3 - 2 line at a spatial resolution of 8 au (0.″14). The CO emission exhibits a bright inner core, a shoulder at r ≈ 70 au, and a prominent break in slope at r …

2018 The Astrophysical Journal
Gaia 157
“Super-deblended” Dust Emission in Galaxies. II. Far-IR to (Sub)millimeter Photometry and High-redshift Galaxy Candidates in the Full COSMOS Field
DOI: 10.3847/1538-4357/aad4af Bibcode: 2018ApJ...864...56J

Calabrò, Antonello; Dickinson, Mark; Daddi, Emanuele +17 more

We present a “super-deblended” far-infrared (FIR) to (sub)millimeter photometric catalog in the Cosmic Evolution Survey (COSMOS), prepared with the method recently developed by Liu et al., with key adaptations. We obtain point-spread function fitting photometry at fixed prior positions including 88,008 galaxies detected in VLA 1.4, 3 GHz, and/or M…

2018 The Astrophysical Journal
Herschel 156
The Eccentric Cavity, Triple Rings, Two-armed Spirals, and Double Clumps of the MWC 758 Disk
DOI: 10.3847/1538-4357/aac6cb Bibcode: 2018ApJ...860..124D

Dong, Ruobing; Tamura, Motohide; Wisniewski, John +15 more

Spatially resolved structures in protoplanetary disks hint at unseen planets. Previous imaging observations of the transitional disk around MWC 758 revealed an inner cavity, a ring-like outer disk, emission clumps, and spiral arms, all possibly generated by companions. We present ALMA dust continuum observations of MWC 758 at 0.87 mm wavelength wi…

2018 The Astrophysical Journal
Gaia 155
Sun-to-Earth MHD Simulation of the 2000 July 14 “Bastille Day” Eruption
DOI: 10.3847/1538-4357/aab36d Bibcode: 2018ApJ...856...75T

Downs, Cooper; Riley, Pete; Linker, Jon A. +6 more

Solar eruptions are the main driver of space-weather disturbances at Earth. Extreme events are of particular interest, not only because of the scientific challenges they pose, but also because of their possible societal consequences. Here we present a magnetohydrodynamic (MHD) simulation of the 2000 July 14 “Bastille Day” eruption, which produced …

2018 The Astrophysical Journal
SOHO 153
Size-Luminosity Relations and UV Luminosity Functions at z = 6-9 Simultaneously Derived from the Complete Hubble Frontier Fields Data
DOI: 10.3847/1538-4357/aaa6cf Bibcode: 2018ApJ...855....4K

Ouchi, Masami; Shimasaku, Kazuhiro; Oguri, Masamune +3 more

We construct z ∼ 6-7, 8, and 9 faint Lyman break galaxy samples (334, 61, and 37 galaxies, respectively) with accurate size measurements with the software glafic from the complete Hubble Frontier Fields (HFF) cluster and parallel fields data. These are the largest samples hitherto and reach down to the faint ends of recently obtained deep luminosi…

2018 The Astrophysical Journal
eHST 151
The Large-scale Structure of the Halo of the Andromeda Galaxy. II. Hierarchical Structure in the Pan-Andromeda Archaeological Survey
DOI: 10.3847/1538-4357/aae8e7 Bibcode: 2018ApJ...868...55M

Lewis, Geraint F.; Dotter, Aaron; Babul, Arif +29 more

The Pan-Andromeda Archaeological Survey is a survey of >400 square degrees centered on the Andromeda (M31) and Triangulum (M33) galaxies that has provided the most extensive panorama of an L galaxy group to large projected galactocentric radii. Here, we collate and summarize the current status of our knowledge of the substructures …

2018 The Astrophysical Journal
Gaia 151
The Disk Substructures at High Angular Resolution Project (DSHARP). III. Spiral Structures in the Millimeter Continuum of the Elias 27, IM Lup, and WaOph 6 Disks
DOI: 10.3847/2041-8213/aaf7a0 Bibcode: 2018ApJ...869L..43H

Hughes, A. Meredith; Wilner, David J.; Andrews, Sean M. +13 more

We present an analysis of Atacama Large Millimeter/submillimeter Array 1.25 mm continuum observations of spiral structures in three protoplanetary disks from the Disk Substructures at High Angular Resolution Project. The disks around Elias 27, IM Lup, and WaOph 6 were observed at a resolution of ∼40-60 mas (∼6-7 au). All three disks feature m = 2 …

2018 The Astrophysical Journal
Gaia 151
One Large Blob and Many Streams Frosting the nearby Stellar Halo in Gaia DR2
DOI: 10.3847/2041-8213/aac882 Bibcode: 2018ApJ...860L..11K

Helmi, Amina; Veljanoski, Jovan; Koppelman, Helmer

We explore the phase-space structure of nearby halo stars identified kinematically from the Gaia second data release (DR2). We focus on their distribution in velocity and in “integrals of motion” space, as well as on their photometric properties. Our sample of stars selected to be moving at a relative velocity of at least 210 km s-1, wi…

2018 The Astrophysical Journal
Gaia 150