Search Publications

Measuring Radial Orbit Migration in the Galactic Disk
DOI: 10.3847/1538-4357/aadba5 Bibcode: 2018ApJ...865...96F

Ting, Yuan-Sen; Hogg, David W.; Rix, Hans-Walter +2 more

We develop and apply a model to quantify the global efficiency of radial orbit migration among stars in the Milky Way disk. This model parameterizes the possible star formation and enrichment histories and radial birth profiles, and combines them with a migration model that relates present-day orbital radii to birth radii through a Gaussian probab…

2018 The Astrophysical Journal
Gaia 143
Evidence for Pulsar-like Emission Components in the Broadband ULX Sample
DOI: 10.3847/1538-4357/aab610 Bibcode: 2018ApJ...856..128W

Harrison, F. A.; Stern, D.; Fabian, A. C. +7 more

We present broadband X-ray analyses of a sample of bright ultraluminous X-ray sources (ULX) with the goal of investigating the spectral similarity of this population to the known ULX pulsars, M82 X-2, NGC 7793 P13, and NGC 5907 ULX. We perform a phase-resolved analysis of the broadband XMM-Newton+NuSTAR data set of NGC 5907 ULX, finding that the p…

2018 The Astrophysical Journal
XMM-Newton 142
“Super-deblended” Dust Emission in Galaxies. I. The GOODS-North Catalog and the Cosmic Star Formation Rate Density out to Redshift 6
DOI: 10.3847/1538-4357/aaa600 Bibcode: 2018ApJ...853..172L

Dickinson, Mark; Inami, Hanae; Daddi, Emanuele +10 more

We present a new technique to measure multi-wavelength “super-deblended” photometry from highly confused images, which we apply to Herschel and ground-based far-infrared (FIR) and (sub-)millimeter (mm) data in the northern field of the Great Observatories Origins Deep Survey. There are two key novelties. First, starting with a large database of de…

2018 The Astrophysical Journal
Herschel eHST 141
The Disk Substructures at High Angular Resolution Project (DSHARP). IX. A High-definition Study of the HD 163296 Planet-forming Disk
DOI: 10.3847/2041-8213/aaf747 Bibcode: 2018ApJ...869L..49I

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

The Atacama Large Millimeter/submillimeter Array observations of protoplanetary disks acquired by the Disk Substructure at High Angular Resolution Project resolve the dust and gas emission on angular scales as small as 3 astronomical units, offering an unprecedented detailed view of the environment where planets form. In this Letter, we present an…

2018 The Astrophysical Journal
Gaia 141
The Missing Satellites of the Magellanic Clouds? Gaia Proper Motions of the Recently Discovered Ultra-faint Galaxies
DOI: 10.3847/1538-4357/aadfee Bibcode: 2018ApJ...867...19K

van der Marel, Roeland P.; Navarro, Julio F.; Sacchi, Elena +7 more

According to LCDM theory, hierarchical evolution occurs on all mass scales, implying that satellites of the Milky Way should also have companions. The recent discovery of ultra-faint dwarf galaxy candidates in close proximity to the Magellanic Clouds provides an opportunity to test this theory. We present proper motion (PM) measurements for 13 of …

2018 The Astrophysical Journal
Gaia 140
The Gould’s Belt Distances Survey (GOBELINS). V. Distances and Kinematics of the Perseus Molecular Cloud
DOI: 10.3847/1538-4357/aada49 Bibcode: 2018ApJ...865...73O

Kounkel, Marina; Rodríguez, Luis F.; Loinard, Laurent +10 more

We derive the distance and structure of the Perseus molecular cloud by combining trigonometric parallaxes from Very Long Baseline Array (VLBA) observations, taken as part of the GOBELINS survey and Gaia Data Release 2. Based on our VLBA astrometry, we obtain a distance of 321 ± 10 pc for IC 348. This is fully consistent with the mean distance of 3…

2018 The Astrophysical Journal
Gaia 137
A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations
DOI: 10.3847/2041-8213/aaad64 Bibcode: 2018ApJ...854L..31C

Covino, S.; D'Avanzo, P.; Lyman, J. D. +25 more

The joint detection of gravitational waves (GWs) and electromagnetic radiation from the binary neutron star (BNS) merger GW170817 has provided unprecedented insight into a wide range of physical processes: heavy element synthesis via the r-process; the production of relativistic ejecta; the equation of state of neutron stars and the nature of the …

2018 The Astrophysical Journal
eHST 137
Spectroscopic Observations of Current Sheet Formation and Evolution
DOI: 10.3847/1538-4357/aaa9b8 Bibcode: 2018ApJ...854..122W

Warren, Harry P.; Doschek, George A.; Ugarte-Urra, Ignacio +3 more

We report on the structure and evolution of a current sheet that formed in the wake of an eruptive X8.3 flare observed at the west limb of the Sun on 2017 September 10. Using observations from the EUV Imaging Spectrometer (EIS) on Hinode and the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory, we find that plasma in the curren…

2018 The Astrophysical Journal
Hinode 137
Dust Attenuation, Bulge Formation, and Inside-out Quenching of Star Formation in Star-forming Main Sequence Galaxies at z ∼ 2
DOI: 10.3847/1538-4357/aabf8b Bibcode: 2018ApJ...859...56T

Wuyts, S.; Förster Schreiber, N. M.; Genzel, R. +10 more

We derive 2D dust attenuation maps at ∼1 kpc resolution from the UV continuum for 10 galaxies on the z ∼ 2 star-forming main sequence (SFMS). Comparison with IR data shows that 9 out of 10 galaxies do not require further obscuration in addition to the UV-based correction, though our sample does not include the most heavily obscured, massive galaxi…

2018 The Astrophysical Journal
eHST 137
Revival of the Magnetar PSR J1622-4950: Observations with MeerKAT, Parkes, XMM-Newton, Swift, Chandra, and NuSTAR
DOI: 10.3847/1538-4357/aab35a Bibcode: 2018ApJ...856..180C

Tasse, C.; Camilo, F.; Stappers, B. +205 more

New radio (MeerKAT and Parkes) and X-ray (XMM-Newton, Swift, Chandra, and NuSTAR) observations of PSR J1622-4950 indicate that the magnetar, in a quiescent state since at least early 2015, reactivated between 2017 March 19 and April 5. The radio flux density, while variable, is approximately 100× larger than during its dormant state. The X-ray flu…

2018 The Astrophysical Journal
XMM-Newton 136