Search Publications

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
Seasonal Evolution on the Nucleus of Comet C/2013 A1 (Siding Spring)
DOI: 10.3847/2041-8205/817/2/L23 Bibcode: 2016ApJ...817L..23L

Samarasinha, Nalin H.; A'Hearn, Michael F.; Bodewits, Dennis +6 more

We observed Comet C/Siding Spring using the Hubble Space Telescope (HST) during its close approach to Mars. The high spatial resolution images obtained through the F689M, F775W, and F845M filters reveal the characteristics of the dust coma. The dust production rate of C/Siding Spring, quantified by Afρ, is 590 ± 30, 640 ± 30, and 670 ± 30 cm in a …

2016 The Astrophysical Journal
eHST 9
Star Formation in Ultraluminous Infrared Galaxies Probed with AKARI Near-infrared Spectroscopy
DOI: 10.3847/1538-4357/833/2/272 Bibcode: 2016ApJ...833..272Y

Nakagawa, Takao; Isobe, Naoki; Shirahata, Mai +1 more

We conducted systematic observations of the H I Brα line (4.05 µm) and the polycyclic aromatic hydrocarbon (PAH) feature (3.3 µm) in 50 nearby (z\lt 0.3) ultraluminous infrared galaxies (ULIRGs) with AKARI. The Brα line is predicted to be the brightest among the H I lines under conditions of high dust extinction ({A}V\gt 15 …

2016 The Astrophysical Journal
AKARI 9
Bayesian Analysis of Two Stellar Populations in Galactic Globular Clusters. II. NGC 5024, NGC 5272, and NGC 6352
DOI: 10.3847/0004-637X/826/1/42 Bibcode: 2016ApJ...826...42W

Jefferys, W. H.; Stenning, D. C.; Wagner-Kaiser, R. +5 more

We use Cycle 21 Hubble Space Telescope (HST) observations and HST archival Advanced Camera for Surveys Treasury observations of Galactic Globular Clusters to find and characterize two stellar populations in NGC 5024 (M53), NGC 5272 (M3), and NGC 6352. For these three clusters, both single and double-population analyses are used to determine a best…

2016 The Astrophysical Journal
eHST 9
From the LIR-T Relation to the Limited Sizes of Dusty Starbursting Regions at High Redshifts
DOI: 10.3847/2041-8205/820/1/L16 Bibcode: 2016ApJ...820L..16Y

Yan, Haojing; Ma, Zhiyuan

Using the far-infrared (IR) data obtained by the Herschel Space Observatory, we study the relation between the IR luminosity (LIR) and the dust temperature (T) of dusty starbursting galaxies at high redshifts (high-z). We focus on the total IR luminosity from the cold-dust component ({L}{IR}({cd)}), whose emission …

2016 The Astrophysical Journal
Herschel 9
Wide Field CO Mapping in the Region of IRAS 19312+1950
DOI: 10.3847/0004-637X/825/1/16 Bibcode: 2016ApJ...825...16N

Zhang, Yong; Hsia, Chih-Hao; Yung, Bosco H. K. +3 more

We report the results of wide field CO mapping in the region of IRAS 19312+1950. This Infrared Astronomical Satellite (IRAS) object exhibits SiO/H2O/OH maser emission, and is embedded in a chemically rich molecular component, the origin of which is still unknown. In order to reveal the entire structure and gas mass of the surrounding mo…

2016 The Astrophysical Journal
AKARI Planck eHST 9