Search Publications

Resolved Kinematics of Runaway and Field OB Stars in the Small Magellanic Cloud
DOI: 10.3847/2041-8213/aae892 Bibcode: 2018ApJ...867L...8O

Lennon, D. J.; Oey, M. S.; Castro, N. +6 more

We use Gaia Data Release 2 proper motions of field OB stars from the Runaways and Isolated O-Type Star Spectroscopic Survey of the Small Magellanic Cloud (SMC) to study the kinematics of runaway stars. The data reveal that the SMC Wing has a systemic peculiar motion relative to the SMC Bar of ({v}α ,{v}δ ) =(62+/- 7,-18+/- 5)…

2018 The Astrophysical Journal
Gaia 38
The Charge State of Polycyclic Aromatic Hydrocarbons across a Reflection Nebula, an H II Region, and a Planetary Nebula
DOI: 10.3847/1538-4357/aabcbe Bibcode: 2018ApJ...858...67B

Boersma, C.; Allamandola, L. J.; Bregman, J.

Low-resolution Spitzer-IRS spectral map data of a reflection nebula (NGC 7023), H II region (M17), and planetary nebula (NGC 40), totaling 1417 spectra, are analyzed using the data and tools available through the NASA Ames PAH IR Spectroscopic Database. The polycyclic aromatic hydrocarbon (PAH) emission is broken down into PAH charge and size subc…

2018 The Astrophysical Journal
eHST 38
Accretion Disk Size Measurement and Time Delays in the Lensed Quasar WFI 2033-4723
DOI: 10.3847/1538-4357/aaed3e Bibcode: 2018ApJ...869..106M

Kochanek, Christopher S.; Bonvin, Vivien; Courbin, Frederic +5 more

We present 13 seasons of R-band photometry of the quadruply lensed quasar WFI 2033-4723 from the 1.3 m SMARTS telescope at CTIO and the 1.2 m Euler Swiss Telescope at La Silla, in which we detect microlensing variability of ∼0.2 mag on a timescale of ∼6 years. Using a Bayesian Monte Carlo technique, we analyze the microlensing signal to obtain a m…

2018 The Astrophysical Journal
eHST 38
Nearby High-speed Stars in Gaia DR2
DOI: 10.3847/1538-4357/aae83e Bibcode: 2018ApJ...868...25B

Geller, Margaret J.; Brown, Warren R.; Kenyon, Scott J. +1 more

We investigate the nature of nearby (10-15 kpc) high-speed stars in the Gaia DR2 archive identified on the basis of parallax, proper motion and radial velocity. Together with a consideration of their kinematic, orbital, and photometric properties, we develop a novel strategy for evaluating whether high-speed stars are statistical outliers of the b…

2018 The Astrophysical Journal
Gaia 38
On the Stellar Velocity Distribution in the Solar Neighborhood in Light of Gaia DR2
DOI: 10.3847/2041-8213/aad804 Bibcode: 2018ApJ...863L..37M

Pérez-Villegas, Angeles; Barros, Douglas A.; Michtchenko, Tatiana A. +2 more

The aim of this Letter is to contribute to the understanding of the stellar velocity distribution in the solar neighborhood (SN). We propose that the structures on the U-V planes, known as the moving groups, can be mainly explained by the spiral arms perturbations. The applied model of the Galactic disk and spiral arms, with the parameters defined…

2018 The Astrophysical Journal
Gaia 38
Recoiling Supermassive Black Hole in Changing-look AGN Mrk 1018
DOI: 10.3847/1538-4357/aac77d Bibcode: 2018ApJ...861...51K

Kim, D. -C.; Evans, A. S.; Yoon, Ilsang

The spectral type of Mrk 1018 changed from Type 1.9 to 1 and returned back to 1.9 over a period of 40 years. We have investigated physical mechanisms responsible for the spectral change in Mrk 1018 by analyzing archival spectral and imaging data. Two kinematically distinct broad-line components, blueshifted and redshifted components, are found fro…

2018 The Astrophysical Journal
eHST 38
Parameterizations of Chromospheric Condensations in dG and dMe Model Flare Atmospheres
DOI: 10.3847/1538-4357/aa9d91 Bibcode: 2018ApJ...852...61K

Kowalski, Adam F.; Allred, Joel C.

The origin of the near-ultraviolet and optical continuum radiation in flares is critical for understanding particle acceleration and impulsive heating in stellar atmospheres. Radiative-hydrodynamic (RHD) simulations in 1D have shown that high energy deposition rates from electron beams produce two flaring layers at T ∼ 104 K that develo…

2018 The Astrophysical Journal
IRIS 38
IRIS Observations of Magnetic Interactions in the Solar Atmosphere between Preexisting and Emerging Magnetic Fields. I. Overall Evolution
DOI: 10.3847/1538-4357/aab2a8 Bibcode: 2018ApJ...856..127G

Young, Peter R.; Murabito, Mariarita; Guglielmino, Salvo L. +2 more

We report multiwavelength ultraviolet observations taken with the IRIS satellite, concerning the emergence phase in the upper chromosphere and transition region of an emerging flux region (EFR) embedded in the preexisting field of active region NOAA 12529 in the Sun. IRIS data are complemented by full-disk observations of the Solar Dynamics Observ…

2018 The Astrophysical Journal
Hinode IRIS 37
Statistical Study of Magnetic Nonpotential Measures in Confined and Eruptive Flares
DOI: 10.3847/1538-4357/aac272 Bibcode: 2018ApJ...860...58V

Ravindra, B.; Doddamani, V. H.; Vemareddy, P. +1 more

Using Solar Dynamics Observatory/Helioseismic and Magnetic Imager vector magnetic field observations, we studied the relation between the degree of magnetic non-potentiality with the observed flare/coronal mass ejection (CME) in active regions (ARs). From a sample of 77 flare/CME cases, we found in general that the degree of non-potentiality is po…

2018 The Astrophysical Journal
SOHO 37
HST Grism Observations of a Gravitationally Lensed Redshift 9.5 Galaxy
DOI: 10.3847/1538-4357/aaa9c2 Bibcode: 2018ApJ...854...39H

Hoag, A.; Bradač, M.; Brammer, G. +11 more

We present deep spectroscopic observations of a Lyman break galaxy (LBG) candidate (hereafter MACS1149-JD) at z ∼ 9.5 with the Hubble Space Telescope (HST) WFC3/IR grisms. The grism observations were taken at four distinct position angles, totaling 34 orbits with the G141 grism, although only 19 of the orbits are relatively uncontaminated along th…

2018 The Astrophysical Journal
eHST 37