Search Publications

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
Accretion Disk Reverberation with Hubble Space Telescope Observations of NGC 4593: Evidence for Diffuse Continuum Lags
DOI: 10.3847/1538-4357/aab4f7 Bibcode: 2018ApJ...857...53C

Horne, Keith; Goad, Michael R.; Korista, Kirk T. +4 more

The Seyfert 1 galaxy NGC 4593 was monitored spectroscopically with the Hubble Space Telescope as part of a reverberation mapping campaign that also included Swift, Kepler, and ground-based photometric monitoring. During 2016 July 12-August 6, we obtained 26 spectra across a nearly continuous wavelength range of ∼1150-10000 Å. These were combined w…

2018 The Astrophysical Journal
eHST 135
The MOSDEF Survey: A Stellar Mass-SFR-Metallicity Relation Exists at z ∼ 2.3
DOI: 10.3847/1538-4357/aabcbd Bibcode: 2018ApJ...858...99S

Barro, Guillermo; Siana, Brian; Shapley, Alice E. +15 more

We investigate the nature of the relation among stellar mass, star formation rate, and gas-phase metallicity (the {M}* -SFR-Z relation) at high redshifts using a sample of 260 star-forming galaxies at z ∼ 2.3 from the MOSDEF survey. We present an analysis of the high-redshift {M}* -SFR-Z relation based on several emission-lin…

2018 The Astrophysical Journal
eHST 135
Apocenter Pile-up: Origin of the Stellar Halo Density Break
DOI: 10.3847/2041-8213/aad0ee Bibcode: 2018ApJ...862L...1D

Belokurov, Vasily; Koposov, Sergey E.; Deason, Alis J. +1 more

We measure the orbital properties of halo stars using seven-dimensional information provided by Gaia and the Sloan Digital Sky Survey. A metal-rich population of stars, present in both local main sequence stars and more distant blue horizontal branch stars, have very radial orbits (eccentricity ∼0.9) and apocenters that coincide with the stellar h…

2018 The Astrophysical Journal
Gaia 133
Scaling Relations Associated with Millimeter Continuum Sizes in Protoplanetary Disks
DOI: 10.3847/1538-4357/aadd9f Bibcode: 2018ApJ...865..157A

Wilner, David J.; Andrews, Sean M.; Ansdell, Megan +3 more

We present a combined, homogenized analysis of archival Submillimeter Array (SMA) and Atacama Large Millimeter/submillimeter Array (ALMA) observations of the spatially resolved 340 GHz (870 µm) continuum emission from 105 nearby protoplanetary disks. Building on the previous SMA survey, we infer surface brightness profiles using a simple mod…

2018 The Astrophysical Journal
Gaia 131
The Extended Distribution of Baryons around Galaxies
DOI: 10.3847/1538-4357/aacafe Bibcode: 2018ApJ...862....3B

Bregman, Joel N.; Anderson, Michael E.; Qu, Zhijie +5 more

We summarize and reanalyze observations bearing on missing galactic baryons, where we propose a consistent picture for halo gas in L ≳ L* galaxies. The hot X-ray-emitting halos are detected to 50-70 kpc, where typically M hot(<50 kpc) ∼ 5 × 109 M , and with density n ∝ r -3/2. When extrapolated to R …

2018 The Astrophysical Journal
Planck XMM-Newton eHST 129