Search Publications

Resolving the ISM at the Peak of Cosmic Star Formation with ALMA: The Distribution of CO and Dust Continuum in z ∼ 2.5 Submillimeter Galaxies
DOI: 10.3847/1538-4357/aacffa Bibcode: 2018ApJ...863...56C

Smail, Ian; Brandt, W. N.; Rybak, M. +17 more

We use Atacama Large Millimeter Array (ALMA) observations of four submillimeter galaxies (SMGs) at z ∼ 2-3 to investigate the spatially resolved properties of the interstellar medium (ISM) at scales of 1-5 kpc (0.″1-0.″6). The velocity fields of our sources, traced by the 12CO(J = 3-2) emission, are consistent with disk rotation to the …

2018 The Astrophysical Journal
eHST 113
Determination of Differential Emission Measure from Solar Extreme Ultraviolet Images
DOI: 10.3847/2041-8213/aab436 Bibcode: 2018ApJ...856L..17S

Veronig, Astrid M.; Gan, Weiqun; Cheung, Mark C. M. +5 more

The Atmospheric Imaging Assembly (AIA) on board the Solar Dynamic Observatory (SDO) has been providing high-cadence, high-resolution, full-disk UV-visible/extreme ultraviolet (EUV) images since 2010, with the best time coverage among all the solar missions. A number of codes have been developed to extract plasma differential emission measures (DEM…

2018 The Astrophysical Journal
Hinode 110
The R-Process Alliance: First Release from the Northern Search for r-process-enhanced Metal-poor Stars in the Galactic Halo
DOI: 10.3847/1538-4357/aae9df Bibcode: 2018ApJ...868..110S

Grebel, Eva K.; Steinmetz, Matthias; Beers, Timothy C. +26 more

This paper presents the detailed abundances and r-process classifications of 126 newly identified metal-poor stars as part of an ongoing collaboration, the R-Process Alliance. The stars were identified as metal-poor candidates from the RAdial Velocity Experiment (RAVE) and were followed up at high spectral resolution (R ∼ 31,500) with the 3.5 m te…

2018 The Astrophysical Journal
Gaia 109
The Kepler Light Curves of AGN: A Detailed Analysis
DOI: 10.3847/1538-4357/aab88d Bibcode: 2018ApJ...857..141S

Howell, Steve B.; Gelino, Dawn M.; Boyd, Patricia T. +3 more

We present a comprehensive analysis of 21 light curves of Type 1 active galactic nuclei (AGN) from the Kepler spacecraft. First, we describe the necessity and development of a customized pipeline for treating Kepler data of stochastically variable sources like AGN. We then present the light curves, power spectral density functions (PSDs), and flux…

2018 The Astrophysical Journal
XMM-Newton 109
The Disk Substructures at High Angular Resolution Project (DSHARP). IV. Characterizing Substructures and Interactions in Disks around Multiple Star Systems
DOI: 10.3847/2041-8213/aaf746 Bibcode: 2018ApJ...869L..44K

Wilner, David J.; Andrews, Sean M.; Guzmán, Viviana V. +11 more

To characterize the substructures induced in protoplanetary disks by the interaction between stars in multiple systems, we study the 1.25 mm continuum and the 12CO(J = 2-1) spectral line emission of the triple systems HT Lup and AS 205, at scales of ≈5 au, as part of the “Disk Substructures at High Angular Resolution Project” (DSHARP). …

2018 The Astrophysical Journal
Gaia 107
The MAVERIC Survey: Still No Evidence for Accreting Intermediate-mass Black Holes in Globular Clusters
DOI: 10.3847/1538-4357/aac9b9 Bibcode: 2018ApJ...862...16T

Strader, Jay; Maccarone, Thomas J.; Seth, Anil C. +8 more

We present the results of an ultradeep, comprehensive radio continuum survey for the accretion signatures of intermediate-mass black holes (IMBHs) in globular clusters (GCs). The sample, imaged with the Karl G. Jansky Very Large Array and the Australia Telescope Compact Array, comprises 50 Galactic GCs. No compelling evidence for an IMBH is found …

2018 The Astrophysical Journal
eHST 107
A Survey of Atomic Carbon [C I] in High-redshift Main-sequence Galaxies
DOI: 10.3847/1538-4357/aaeb88 Bibcode: 2018ApJ...869...27V

Dickinson, Mark E.; Lee, Min-Young; Daddi, Emanuele +15 more

We present the first results of an Atacama Large Millimeter Array survey of the lower fine-structure line of atomic carbon [C I] {(}3{P}1 {--}{}3{P}0) in far-infrared-selected galaxies on the main sequence at z ∼ 1.2 in the COSMOS field. We compare our sample with a comprehensive compilation of data avai…

2018 The Astrophysical Journal
Herschel 107
Multiple Disk Gaps and Rings Generated by a Single Super-Earth. II. Spacings, Depths, and Number of Gaps, with Application to Real Systems
DOI: 10.3847/1538-4357/aadadd Bibcode: 2018ApJ...866..110D

Dong, Ruobing; Li, Hui; Chiang, Eugene +1 more

The Atacama Large Millimeter/submillimeter Array (ALMA) has found multiple dust gaps and rings in a number of protoplanetary disks in continuum emission at millimeter wavelengths. The origin of such structures is under debate. Recently, we documented how one super-Earth planet can open multiple (up to five) dust gaps in a disk with low viscosity (…

2018 The Astrophysical Journal
Gaia 106
GRB 170817A Associated with GW170817: Multi-frequency Observations and Modeling of Prompt Gamma-Ray Emission
DOI: 10.3847/2041-8213/aaa2f6 Bibcode: 2018ApJ...852L..30P

Lyutikov, M.; Minaev, P. Yu.; Pozanenko, A. S. +7 more

We present our observations of electromagnetic transients associated with GW170817/GRB 170817A using optical telescopes of Chilescope observatory and Big Scanning Antenna (BSA) of Pushchino Radio Astronomy Observatory at 110 MHz. The Chilescope observatory detected an optical transient of ∼19m on the third day in the outskirts of the ga…

2018 The Astrophysical Journal
INTEGRAL 106
Mapping Distances across the Perseus Molecular Cloud Using CO Observations, Stellar Photometry, and Gaia DR2 Parallax Measurements
DOI: 10.3847/1538-4357/aae97c Bibcode: 2018ApJ...869...83Z

Speagle, Joshua S.; Zucker, Catherine; Finkbeiner, Douglas P. +4 more

We present a new technique to determine distances to major star-forming regions across the Perseus Molecular Cloud, using a combination of stellar photometry, astrometric data, and 12CO spectral-line maps. Incorporating the Gaia DR2 parallax measurements when available, we start by inferring the distance and reddening to stars from thei…

2018 The Astrophysical Journal
Gaia 106