Search Publications

Evidence for Intermediate Polars as the Origin of the Galactic Center Hard X-ray Emission
DOI: 10.3847/0004-637X/826/2/160 Bibcode: 2016ApJ...826..160H

Hailey, Charles J.; Mori, Kaya; Zhang, Shuo +14 more

Recently, unresolved hard (20-40 keV) X-ray emission has been discovered within the central 10 pc of the Galaxy, possibly indicating a large population of intermediate polars (IPs). Chandra and XMM-Newton measurements in the surrounding ∼50 pc imply a much lighter population of IPs with < {M}{{WD}}> ≈ 0.5{M}. Here we …

2016 The Astrophysical Journal
INTEGRAL XMM-Newton 62
Dissecting the High-z Interstellar Medium through Intensity Mapping Cross-correlations
DOI: 10.3847/1538-4357/833/2/153 Bibcode: 2016ApJ...833..153S

Lagache, Guilaine; Doré, Olivier; Serra, Paolo

We explore the detection, with upcoming spectroscopic surveys, of three-dimensional power spectra of emission line fluctuations produced in different phases of the interstellar medium (ISM) by forbidden transitions of ionized carbon [C II] (157.7 µm), ionized nitrogen [N II] (121.9 and 205.2 µm), and neutral oxygen [O I] (145.5 µ…

2016 The Astrophysical Journal
ISO 62
A Case Against Spinning PAHs as the Source of the Anomalous Microwave Emission
DOI: 10.3847/0004-637X/827/1/45 Bibcode: 2016ApJ...827...45H

Meisner, Aaron M.; Draine, B. T.; Hensley, Brandon S.

We employ an all-sky map of the anomalous microwave emission (AME) produced by component separation of the microwave sky to study correlations between the AME and Galactic dust properties. We find that while the AME is highly correlated with all tracers of dust emission, the best predictor of the AME strength is the dust radiance. Fluctuations in …

2016 The Astrophysical Journal
Planck 62
NuSTAR Hard X-Ray Survey of the Galactic Center Region. II. X-Ray Point Sources
DOI: 10.3847/0004-637X/825/2/132 Bibcode: 2016ApJ...825..132H

Hailey, Charles J.; Mori, Kaya; Giommi, Paolo +41 more

We present the first survey results of hard X-ray point sources in the Galactic Center (GC) region by NuSTAR. We have discovered 70 hard (3-79 keV) X-ray point sources in a 0.6 deg{}2 region around Sgr A* with a total exposure of 1.7 Ms, and 7 sources in the Sgr B2 field with 300 ks. We identify clear Chandra counterparts for 58 NuSTAR …

2016 The Astrophysical Journal
XMM-Newton 62
Living with a Red Dwarf: Rotation and X-Ray and Ultraviolet Properties of the Halo Population Kapteyn's Star
DOI: 10.3847/0004-637X/821/2/81 Bibcode: 2016ApJ...821...81G

Guinan, Edward F.; Engle, Scott G.; Durbin, Allyn

As part of Villanova's Living with a Red Dwarf program, we have obtained UV, X-ray, and optical data of the Population II red dwarf -- Kapteyn's Star. Kapteyn's Star is noteworthy for its large proper motions and high radial velocity of ∼+245 km s-1. As the nearest Pop II red dwarf, it serves as an old age anchor for calibrating activit…

2016 The Astrophysical Journal
IUE eHST 61
The Runaways and Isolated O-Type Star Spectroscopic Survey of the SMC (RIOTS4)
DOI: 10.3847/0004-637X/817/2/113 Bibcode: 2016ApJ...817..113L

Oey, M. S.; Parker, J. Wm.; Kiminki, D. C. +4 more

We present the Runaways and Isolated O-Type Star Spectroscopic Survey of the SMC (RIOTS4), a spatially complete survey of uniformly selected field OB stars that covers the entire star-forming body of the Small Magellanic Cloud (SMC). Using the IMACS (Inamori-Magellan Areal Camera and Spectrograph) multislit spectrograph and MIKE (Magellan Inamori …

2016 The Astrophysical Journal
eHST 61
Relationship of EUV Irradiance Coronal Dimming Slope and Depth to Coronal Mass Ejection Speed and Mass
DOI: 10.3847/0004-637X/830/1/20 Bibcode: 2016ApJ...830...20M

Vourlidas, Angelos; Colaninno, Robin C.; Woods, Thomas N. +3 more

Extreme ultraviolet (EUV) coronal dimmings are often observed in response to solar eruptive events. These phenomena can be generated via several different physical processes. For space weather, the most important of these is the temporary void left behind by a coronal mass ejection (CME). Massive, fast CMEs tend to leave behind a darker void that …

2016 The Astrophysical Journal
SOHO 61
The SCUBA-2 Cosmology Legacy Survey: Multiwavelength Counterparts to 103 Submillimeter Galaxies in the UKIDSS-UDS Field
DOI: 10.3847/0004-637X/820/2/82 Bibcode: 2016ApJ...820...82C

Zavala, Jorge A.; Smail, Ian; Conselice, Christopher J. +20 more

We present multiwavelength identifications for the counterparts of 1088 submillimeter sources detected at 850 µm in the SCUBA-2 Cosmology Legacy Survey study of the UKIRT Infrared Deep Sky Survey-Ultra-Deep Survey (UDS) field. By utilizing an Atacama Large Millimeter Array (ALMA) pilot study on a subset of our bright SCUBA-2 sample as a trai…

2016 The Astrophysical Journal
Herschel 61
Detection of a Possible X-Ray Quasi-periodic Oscillation in the Active Galactic Nucleus 1H 0707-495
DOI: 10.3847/2041-8205/819/2/L19 Bibcode: 2016ApJ...819L..19P

Yuan, Weimin; Zhang, Shuang-Nan; Pan, Hai-Wu +4 more

The quasi-periodic oscillation (QPO) detected in the X-ray radiation of black hole X-ray binaries (BHXBs) is thought to originate from dynamical processes in close vicinity of black holes (BHs), and thus carries important physical information therein. Such a feature is extremely rare in active galactic nuclei (AGNs) with supermassive BHs. Here we …

2016 The Astrophysical Journal
XMM-Newton 61
The Panchromatic Hubble Andromeda Treasury. XV. The BEAST: Bayesian Extinction and Stellar Tool
DOI: 10.3847/0004-637X/826/2/104 Bibcode: 2016ApJ...826..104G

Bell, Eric F.; Skillman, Evan D.; Williams, Benjamin F. +17 more

We present the Bayesian Extinction And Stellar Tool (BEAST), a probabilistic approach to modeling the dust extinguished photometric spectral energy distribution of an individual star while accounting for observational uncertainties common to large resolved star surveys. Given a set of photometric measurements and an observational uncertainty model…

2016 The Astrophysical Journal
eHST 60