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Short versus Long and Collapsars versus Non-collapsars: A Quantitative Classification of Gamma-Ray Bursts
DOI: 10.1088/0004-637X/764/2/179 Bibcode: 2013ApJ...764..179B

Piran, Tsvi; Bromberg, Omer; Nakar, Ehud +1 more

Gamma-ray bursts (GRBs) are traditionally divided into long and short according to their durations (lg2 s). It was generally believed that this reflects a different physical origin: collapsars (long) and non-collapsars (short). We have recently shown that the duration distribution of collapsars is flat, namely, independent of the duration, at shor…

2013 The Astrophysical Journal
INTEGRAL 207
A Comprehensive Analysis of Fermi Gamma-Ray Burst Data. III. Energy-dependent T 90 Distributions of GBM GRBs and Instrumental Selection Effect on Duration Classification
DOI: 10.1088/0004-637X/763/1/15 Bibcode: 2013ApJ...763...15Q

Lin, Lin; Zhang, Bing; Liang, En-Wei +8 more

The durations (T 90) of 315 gamma-ray bursts (GRBs) detected with Fermi/GBM (8-1000 keV) up to 2011 September are calculated using the Bayesian Block method. We compare the T 90 distributions between this sample and those derived from previous/current GRB missions. We show that the T 90 distribution of this GRB sam…

2013 The Astrophysical Journal
INTEGRAL 103
Distribution of High-mass X-Ray Binaries in the Milky Way
DOI: 10.1088/0004-637X/764/2/185 Bibcode: 2013ApJ...764..185C

Coleiro, Alexis; Chaty, Sylvain

Observations of the high-energy sky, particularly with the INTEGRAL satellite, have quadrupled the number of supergiant X-ray binaries observed in the Galaxy and revealed new populations of previously hidden high-mass X-ray binaries (HMXBs), raising new questions about their formation and evolution. The number of detected HMXBs of different types …

2013 The Astrophysical Journal
INTEGRAL 77
The Smooth Cyclotron Line in Her X-1 as Seen with Nuclear Spectroscopic Telescope Array
DOI: 10.1088/0004-637X/779/1/69 Bibcode: 2013ApJ...779...69F

Hailey, Charles J.; Fürst, Felix; Klochkov, Dmitry +17 more

Her X-1, one of the brightest and best studied X-ray binaries, shows a cyclotron resonant scattering feature (CRSF) near 37 keV. This makes it an ideal target for a detailed study with the Nuclear Spectroscopic Telescope Array (NuSTAR), taking advantage of its excellent hard X-ray spectral resolution. We observed Her X-1 three times, coordinated w…

2013 The Astrophysical Journal
INTEGRAL Suzaku 59
Superorbital Periodic Modulation in Wind-accretion High-mass X-Ray Binaries from Swift Burst Alert Telescope Observations
DOI: 10.1088/0004-637X/778/1/45 Bibcode: 2013ApJ...778...45C

Corbet, Robin H. D.; Krimm, Hans A.

We report the discovery using data from the Swift-Burst Alert Telescope (BAT) of superorbital modulation in the wind-accretion supergiant high-mass X-ray binaries 4U 1909+07 (= X 1908+075), IGR J16418-4532, and IGR J16479-4514. Together with already known superorbital periodicities in 2S 0114+650 and IGR J16493-4348, the systems exhibit a monotoni…

2013 The Astrophysical Journal
INTEGRAL 56
An Accretion Model for the Anomalous X-Ray Pulsar 4U 0142+61
DOI: 10.1088/0004-637X/764/1/49 Bibcode: 2013ApJ...764...49T

Zezas, A.; Dennerl, K.; Trümper, J. E. +2 more

We propose that the quiescent emission of anomalous X-ray pulsars/soft gamma-ray repeaters (AXPs/SGRs) is powered by accretion from a fallback disk, requiring magnetic dipole fields in the range 1012-1013 G, and that the luminous hard tails of their X-ray spectra are produced by bulk-motion Comptonization in the radiative sho…

2013 The Astrophysical Journal
INTEGRAL 48
Time-dependent Modeling of Pulsar Wind Nebulae
DOI: 10.1088/0004-637X/773/2/139 Bibcode: 2013ApJ...773..139V

Tibolla, O.; Ferreira, S. E. S.; Kaufmann, S. +1 more

A spatially independent model that calculates the time evolution of the electron spectrum in a spherically expanding pulsar wind nebula (PWN) is presented, allowing one to make broadband predictions for the PWN's non-thermal radiation. The source spectrum of electrons injected at the termination shock of the PWN is chosen to be a broken power law.…

2013 The Astrophysical Journal
INTEGRAL 47
Polarimetry in the Hard X-Ray Domain with INTEGRAL SPI
DOI: 10.1088/0004-637X/769/2/137 Bibcode: 2013ApJ...769..137C

Clark, D. J.; Jourdain, E.; Roques, J. P. +1 more

We present recent improvements in polarization analysis with the INTEGRAL SPI data. The SPI detector plane consists of 19 independent Ge crystals and can operate as a polarimeter. The anisotropy characteristics of Compton diffusions can provide information on the polarization parameters of the incident flux. By including the physics of the polariz…

2013 The Astrophysical Journal
INTEGRAL 41
An Archival Chandra and XMM-Newton Survey of Type 2 Quasars
DOI: 10.1088/0004-637X/777/1/27 Bibcode: 2013ApJ...777...27J

Heckman, Timothy; Zakamska, Nadia L.; Ptak, Andrew +1 more

In order to investigate obscuration in high-luminosity type 2 active galactic nuclei (AGNs), we analyzed Chandra and XMM-Newton archival observations for 71 type 2 quasars detected at 0.05 < z < 0.73, which were selected based on their [O III] λ5007 emission lines. For 54 objects with good spectral fits, the observed hard X-ray luminosity ra…

2013 The Astrophysical Journal
INTEGRAL XMM-Newton 37
Rapid Gamma-Ray Flux Variability during the 2013 March Crab Nebula Flare
DOI: 10.1088/2041-8205/775/2/L37 Bibcode: 2013ApJ...775L..37M

Cheung, C. C.; Grove, J. E.; Hays, E. +5 more

We report on a bright flare in the Crab Nebula detected by the Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope. The period of significantly increased luminosity occurred in 2013 March and lasted for approximately two weeks. During this period, we observed flux variability on timescales of approximately 5 hr. The combined ph…

2013 The Astrophysical Journal
INTEGRAL 37