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Variations of the ISM Compactness Across the Main Sequence of Star Forming Galaxies: Observations and Simulations
DOI: 10.3847/0004-637X/817/1/76 Bibcode: 2016ApJ...817...76M

Zezas, A.; Groves, B.; Ashby, M. L. N. +7 more

The majority of star-forming galaxies follow a simple empirical correlation in the star formation rate (SFR) versus stellar mass (M*) plane, of the form {{SFR}}\propto {M}*α , usually referred to as the star formation main sequence (MS). The physics that sets the properties of the MS is currently a subject of debat…

2016 The Astrophysical Journal
Herschel 10
NuSTAR Observations of Magnetar 1E 1048.1-5937
DOI: 10.3847/0004-637X/831/1/80 Bibcode: 2016ApJ...831...80Y

Yang, C.; Guillot, S.; Kaspi, V. M. +5 more

We report on simultaneous Nuclear Spectroscopic Telescope Array (NuSTAR) and XMM-Newton observations of the magnetar 1E 1048.1-5937, along with Rossi X-ray Timing Explorer (RXTE) data for the same source. The NuSTAR data provide a clear detection of this magnetar’s persistent emission up to 20 keV. We detect a previously unreported small secondary…

2016 The Astrophysical Journal
XMM-Newton 10
Testing Relativistic Reflection and Resolving Outflows in PG 1211+143 with XMM-Newton and NuSTAR
DOI: 10.3847/0004-637X/831/2/201 Bibcode: 2016ApJ...831..201L

Vaughan, S.; Reeves, J. N.; Pounds, K. +1 more

We analyze the broad-band X-ray spectrum (0.3-50 keV) of the luminous Seyfert 1/quasar PG 1211+143—the archetypal source for high-velocity X-ray outflows—using near-simultaneous XMM-Newton and NuSTAR observations. We compare pure relativistic reflection models with a model including the strong imprint of photoionized emission and absorption from a…

2016 The Astrophysical Journal
XMM-Newton 10
Constraining White Dwarf Structure and Neutrino Physics in 47 Tucanae
DOI: 10.3847/0004-637X/821/1/27 Bibcode: 2016ApJ...821...27G

Kalirai, J. S.; Heyl, J.; Tremblay, P. E. +2 more

We present a robust statistical analysis of the white dwarf cooling sequence in 47 Tucanae. We combine Hubble Space Telescope UV and optical data in the core of the cluster, Modules for Experiments in Stellar Evolution (MESA) white dwarf cooling models, white dwarf atmosphere models, artificial star tests, and a Markov Chain Monte Carlo sampling m…

2016 The Astrophysical Journal
eHST 10
Multi-wavelength Observations of a Subarcsecond Penumbral Transient Brightening Event
DOI: 10.3847/0004-637X/823/1/60 Bibcode: 2016ApJ...823...60B

Su, J. T.; Cao, W. D.; Deng, Y. Y. +3 more

We report a subarcsecond penumbral transient brightening event with the high-spatial resolution observations from the 1.6 m New Solar Telescope (NST), Interface Region Imaging Spectrograph (IRIS), and the Solar Dynamics Observatory. The transient brightening, whose thermal energy is in the range of nanoflares, has signatures in the chromosphere, t…

2016 The Astrophysical Journal
IRIS 10
Strong-lensing Analysis of the Powerful Lensing Cluster MACS J2135.2-0102 (z = 0.33)
DOI: 10.3847/0004-637X/833/1/25 Bibcode: 2016ApJ...833...25Z

Broadhurst, Tom; Zitrin, Adi

We present a light-traces-mass (LTM) strong-lensing model of the massive lensing cluster MACS J2135.2-0102 (z = 0.33 hereafter MACS2135), known in part for hosting the cosmic eye galaxy lens. MACS2135 is also known to multiply lens a z = 2.3 sub-millimeter galaxy near the brightest cluster galaxy (BCG), as well as a prominent, triply imaged system…

2016 The Astrophysical Journal
eHST 9
Redefining the Boundaries of Interplanetary Coronal Mass Ejections from Observations at the Ecliptic Plane
DOI: 10.3847/0004-637X/828/1/11 Bibcode: 2016ApJ...828...11C

Guerrero, A.; Cid, C.; Saiz, E. +1 more

On 2015 January 6-7, an interplanetary coronal mass ejection (ICME) was observed at L1. This event, which can be associated with a weak and slow coronal mass ejection, allows us to discuss the differences between the boundaries of the magnetic cloud and the compositional boundaries. A fast stream from a solar coronal hole surrounding this ICME off…

2016 The Astrophysical Journal
PROBA-2 SOHO 9
Breakout Reconnection Observed by the TESIS EUV Telescope
DOI: 10.3847/0004-637X/816/2/90 Bibcode: 2016ApJ...816...90R

Reva, A. A.; Ulyanov, A. S.; Kuzin, S. V. +1 more

We present experimental evidence of the coronal mass ejection (CME) breakout reconnection, observed by the TESIS EUV telescope. The telescope could observe solar corona up to 2 R from the Sun center in the Fe 171 Å line. Starting from 2009 April 8, TESIS observed an active region (AR) that had a quadrupolar structure with an X-point 0.…

2016 The Astrophysical Journal
SOHO 9
Suprathermal Electrons in Titan’s Sunlit Ionosphere: Model-Observation Comparisons
DOI: 10.3847/0004-637X/826/2/131 Bibcode: 2016ApJ...826..131V

Coates, A. J.; Wahlund, J. -E.; Edberg, N. J. T. +8 more

The dayside ionosphere of the Saturnian satellite Titan is generated mainly from photoionization of N2 and CH4. We compare model-derived suprathermal electron intensities with spectra measured by the Cassini Plasma Spectrometer/Electron Spectrometer (CAPS/ELS) in Titan's sunlit ionosphere (altitudes of 970-1250 km) focusing o…

2016 The Astrophysical Journal
Cassini 9
Ion injection at Quasi-parallel Shocks Seen by the Cluster Spacecraft
DOI: 10.3847/2041-8205/817/1/L4 Bibcode: 2016ApJ...817L...4J

Dandouras, I.; Vaivads, A.; Khotyaintsev, Yu. V. +2 more

Collisionless shocks in space plasma are known to be capable of accelerating ions to very high energies through diffusive shock acceleration (DSA). This process requires an injection of suprathermal ions, but the mechanisms producing such a suprathermal ion seed population are still not fully understood. We study acceleration of solar wind ions re…

2016 The Astrophysical Journal
Cluster 9