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The Grism Lens-Amplified Survey from Space (GLASS). V. Extent and Spatial Distribution of Star Formation in z ~ 0.5 Cluster Galaxies
DOI: 10.1088/0004-637X/814/2/161 Bibcode: 2015ApJ...814..161V

Fontana, Adriano; Pentericci, Laura; Schmidt, Kasper B. +14 more

We present the first study of the spatial distribution of star formation in z ∼ 0.5 cluster galaxies. The analysis is based on data taken with the Wide Field Camera 3 as part of the Grism Lens-Amplified Survey from Space (GLASS). We illustrate the methodology by focusing on two clusters (MACS 0717.5+3745 and MACS 1423.8+2404) with different morpho…

2015 The Astrophysical Journal
eHST 19
Physical Conditions in the X-Ray Emission-line Gas in NGC 1068
DOI: 10.1088/0004-637X/798/1/53 Bibcode: 2015ApJ...798...53K

Turner, T. J.; Kraemer, S. B.; Crenshaw, D. Michael +2 more

We present a detailed, photoionization modeling analysis of XMM-Newton/Reflection Grating Spectrometer observations of the Seyfert 2 galaxy NGC 1068. The spectrum, previously analyzed by Kinkhabwala et al., reveals a myriad of soft X-ray emission lines, including those from H- and He-like carbon, nitrogen, oxygen, and neon, and M- and L-shell iron…

2015 The Astrophysical Journal
XMM-Newton 19
Temperature and Electron Density Diagnostics of a Candle-flame-shaped Flare
DOI: 10.1088/0004-637X/800/1/54 Bibcode: 2015ApJ...800...54G

Longcope, D. W.; McKenzie, D. E.; Plowman, J. E. +2 more

Candle-flame-shaped flares are archetypical structures that provide indirect evidence of magnetic reconnection. A flare resembling Tsuneta's famous 1992 candle-flame flare occurred on 2011 January 28; we present its temperature and electron density diagnostics. This flare was observed with Solar Dynamics Observatory/Atmospheric Imaging Assembly (S…

2015 The Astrophysical Journal
Hinode 19
Enhancement of the 6.4 keV Line in the Inner Galactic Ridge: Proton-induced Fluorescence?
DOI: 10.1088/2041-8205/807/1/L10 Bibcode: 2015ApJ...807L..10N

Koyama, K.; Tanaka, T.; Fukui, Y. +7 more

A common idea for the origin of the Galactic diffuse X-ray emission, particularly that of the iron lines from neutral and highly ionized atoms, is a superposition of many cataclysmic variables and coronally active binaries. In this scenario, the flux should symmetrically distribute between the east and west on the plane with respect to Sagittarius…

2015 The Astrophysical Journal
Suzaku 19
The Three-dimensional Evolution of Ion-scale Current Sheets: Tearing and Drift-kink Instabilities in the Presence of Proton Temperature Anisotropy
DOI: 10.1088/0004-637X/802/1/4 Bibcode: 2015ApJ...802....4G

Matteini, L.; Burgess, D.; Gingell, P. W.

We present the first three-dimensional (3D) hybrid simulations of the evolution of ion-scale current sheets, with an investigation of the role of temperature anisotropy and associated kinetic instabilities on the growth of the tearing instability and particle heating. We confirm the ability of the ion cyclotron and firehose instabilities to enhanc…

2015 The Astrophysical Journal
Cluster 19
X-Ray Spectral Residuals in NGC 5408 X-1: Diffuse Emission from Star Formation, or the Signature of a Super-Eddington Wind?
DOI: 10.1088/0004-637X/814/1/73 Bibcode: 2015ApJ...814...73S

Middleton, Matthew J.; Sutton, Andrew D.; Roberts, Timothy P.

If ultraluminous X-ray sources (ULXs) are powered by accretion onto stellar remnant black holes, then many must be accreting at super-Eddington rates. It is predicted that such high accretion rates should give rise to massive, radiatively driven winds. However, observational evidence of a wind, in the form of absorption or emission features, has r…

2015 The Astrophysical Journal
eHST 19
Evidence for (and Against) Progenitor Bias in the Size Growth of Compact Red Galaxies
DOI: 10.1088/0004-637X/798/1/26 Bibcode: 2015ApJ...798...26K

Newman, Jeffrey; Graves, Genevieve; Abraham, Roberto G. +5 more

Most massive, passive galaxies are compact at high redshifts, but similarly compact massive galaxies are rare in the local universe. The most common interpretation of this phenomenon is that massive galaxies have grown in size by a factor of about five since redshift z = 2. An alternative explanation is that recently quenched massive galaxies are …

2015 The Astrophysical Journal
eHST 19
X-Ray Emission from J1446--4701, J1311--3430, and Other Black Widow Pulsars
DOI: 10.1088/0004-637X/814/2/90 Bibcode: 2015ApJ...814...90A

Pavlov, George G.; Garmire, Gordon P.; Arumugasamy, Prakash

We present the results of detailed X-ray analysis of two black-widow pulsars (BWPs), J1446-4701 and J1311-3430. PSR J1446-4701 is a BWP with orbital parameters near the median values of the sample of known BWPs. Its X-ray emission that was detected by XMM-Newton is well characterized by a soft power-law (PL) spectrum (photon index Γ ≈ 3), and it s…

2015 The Astrophysical Journal
XMM-Newton 19
Searches for Millisecond Pulsar Candidates among the Unidentified Fermi Objects
DOI: 10.1088/0004-637X/809/1/68 Bibcode: 2015ApJ...809...68H

Cheng, K. S.; Takata, J.; Kong, A. K. H. +9 more

Here we report the results of searching millisecond pulsar (MSP) candidates from the Fermi LAT second source catalog (2FGL). Seven unassociated γ-ray sources in this catalog are identified as promising MSP candidates based on their γ-ray properties. Through the X-ray analysis, we have detected possible X-ray counterparts, localized to an arcsecond…

2015 The Astrophysical Journal
XMM-Newton 19
The Role of Large Amplitude Upstream Low-frequency Waves in the Generation of Superthermal Ions at a Quasi-parallel Collisionless Shock: Cluster Observations
DOI: 10.1088/0004-637X/808/1/2 Bibcode: 2015ApJ...808....2W

Wang, Shui; Huang, Can; Guo, Fan +3 more

The superthermal ions at a quasi-parallel collisionless shock are considered to be generated during the reformation of the shock. Recently, hybrid simulations of a quasi-parallel shock have shown that during the reformation of a quasi-parallel shock the large-amplitude upstream low-frequency waves can trap the reflected ions at the shock front whe…

2015 The Astrophysical Journal
Cluster 19