Search Publications

Spatio-temporal Dynamics of Sources of Hard X-Ray Pulsations in Solar Flares
DOI: 10.1007/s11207-016-0981-3 Bibcode: 2016SoPh..291.3385K

Zimovets, I. V.; Struminsky, A. B.; Kuznetsov, S. A. +1 more

We present a systematic analysis of the spatio-temporal evolution of sources of hard X-ray (HXR) pulsations in solar flares. We concentrate on disk flares whose impulsive phases are accompanied by a series of more than three successive peaks (pulsations) of HXR emission detected in the RHESSI 50 - 100 keV energy channel with a four-second time cad…

2016 Solar Physics
SOHO 31
Disky Elliptical Galaxies and the Allegedly Over-massive Black Hole in the Compact “ES“ Galaxy NGC 1271
DOI: 10.3847/0004-637X/831/2/132 Bibcode: 2016ApJ...831..132G

Ciambur, Bogdan C.; Graham, Alister W.; Savorgnan, Giulia A. D.

While spiral and lenticular galaxies have large-scale disks extending beyond their bulges, and most local early-type galaxies with 1010 < M */M < 2 × 1011 contain a disk (e.g., ATLAS3D), the early-type galaxies do possess a range of disk sizes. The edge-on, intermediate-scale disk in t…

2016 The Astrophysical Journal
eHST 31
A Soft X-Ray Spectral Episode for the Clocked Burster, GS 1826-24 as Measured by Swift and NuStar
DOI: 10.3847/0004-637X/818/2/135 Bibcode: 2016ApJ...818..135C

Harrison, F. A.; Stern, D.; Zhang, W. W. +12 more

We report on NuSTAR and Swift observations of a soft state of the neutron star low-mass X-ray binary GS 1826-24, commonly known as the “clocked” burster. The transition to the soft state was recorded in 2014 June through an increase of the 2-20 keV source intensity measured by MAXI, simultaneous with a decrease of the 15-50 keV intensity measured …

2016 The Astrophysical Journal
INTEGRAL 31
Scale-dependent Normalized Amplitude and Weak Spectral Anisotropy of Magnetic Field Fluctuations in the Solar Wind Turbulence
DOI: 10.3847/0004-637X/816/1/15 Bibcode: 2016ApJ...816...15W

He, Jiansen; Wang, Xin; Wang, Linghua +2 more

Turbulence in the solar wind was recently reported to be anisotropic, with the average power spectral index close to -2 when sampling parallel to the local mean magnetic field B0 and close to -5/3 when sampling perpendicular to the local B0. This result was widely considered to be observational evidence for the critical balan…

2016 The Astrophysical Journal
Ulysses 31
Multiwavelength study of the flaring activity of Sagittarius A in 2014 February-April
DOI: 10.1051/0004-6361/201527554 Bibcode: 2016A&A...589A.116M

Grosso, N.; Porquet, D.; Eckart, A. +8 more

Context. The supermassive black hole named Sgr A* is located at the dynamical center of the Milky Way. This closest supermassive black hole is known to have a luminosity several orders of magnitude lower than the Eddington luminosity. Flares coming from the Sgr A* environment can be observed in infrared, X-ray, and submillimeter wavelengths, but t…

2016 Astronomy and Astrophysics
XMM-Newton eHST 31
A Herschel View of Protoplanetary Disks in the σ Ori Cluster
DOI: 10.3847/0004-637X/829/1/38 Bibcode: 2016ApJ...829...38M

Calvet, Nuria; Briceño, César; Ali, Babar +6 more

We present new Herschel observations using the Photodetector Array Camera and Spectrometer of 32 T Tauri stars in the young (∼3 Myr) σ Ori cluster. Most of our objects are K and M stars with large excesses at 24 µm. We used irradiated accretion disk models of D’Alessio et al. to compare their spectral energy distributions with our observatio…

2016 The Astrophysical Journal
Herschel 31
Flare-generated Shock Wave Propagation through Solar Coronal Arcade Loops and an Associated Type II Radio Burst
DOI: 10.3847/0004-637X/828/1/28 Bibcode: 2016ApJ...828...28K

Innes, D. E.; Kumar, Pankaj; Cho, Kyung-Suk

This paper presents multiwavelength observations of a flare-generated type II radio burst. The kinematics of the shock derived from the type II burst closely match a fast extreme ultraviolet (EUV) wave seen propagating through coronal arcade loops. The EUV wave was closely associated with an impulsive M1.0 flare without a related coronal mass ejec…

2016 The Astrophysical Journal
Hinode 31
LENSED: a code for the forward reconstruction of lenses and sources from strong lensing observations
DOI: 10.1093/mnras/stw2212 Bibcode: 2016MNRAS.463.3115T

Metcalf, R. Benton; Tessore, Nicolas; Bellagamba, Fabio

Robust modelling of strong lensing systems is fundamental to exploit the information they contain about the distribution of matter in galaxies and clusters. In this work, we present LENSED, a new code which performs forward parametric modelling of strong lenses. LENSED takes advantage of a massively parallel ray-tracing kernel to perform the neces…

2016 Monthly Notices of the Royal Astronomical Society
eHST 31
A New M Dwarf Debris Disk Candidate in a Young Moving Group Discovered with Disk Detective
DOI: 10.3847/2041-8205/830/2/L28 Bibcode: 2016ApJ...830L..28S

Kuchner, Marc J.; Gagné, Jonathan; Wisniewski, John P. +14 more

We used the Disk Detective citizen science project and the BANYAN II Bayesian analysis tool to identify a new candidate member of a nearby young association with infrared excess. WISE J080822.18-644357.3, an M5.5-type debris disk system with significant excess at both 12 and 22 µm, is a likely member (∼ 90 % BANYAN II probability) of the ∼45…

2016 The Astrophysical Journal
Gaia 31
Herschel far-infrared photometry of the Swift Burst Alert Telescope active galactic nuclei sample of the local universe - II. SPIRE observations
DOI: 10.1093/mnras/stv2828 Bibcode: 2016MNRAS.456.3335S

Mushotzky, Richard F.; Cowie, Lennox L.; Barger, Amy J. +3 more

We present far-infrared (FIR) and submillimetre photometry from the Herschel Space Observatory's Spectral and Photometric Imaging Receiver (SPIRE) for 313 nearby (z < 0.05) active galactic nuclei (AGN). We selected AGN from the 58 month Swift Burst Alert Telescope (BAT) catalogue, the result of an all-sky survey in the 14-195 keV energy band, a…

2016 Monthly Notices of the Royal Astronomical Society
Herschel Planck 31