Search Publications

Photolytic Hazes in the Atmosphere of 51 Eri b
DOI: 10.3847/0004-637X/824/2/137 Bibcode: 2016ApJ...824..137Z

Morley, C. V.; Zahnle, K.; Moses, J. I. +1 more

We use a 1D model to address photochemistry and possible haze formation in the irradiated warm Jupiter, 51 Eridani b. The intended focus was to be carbon, but sulfur photochemistry turns out to be important. The case for organic photochemical hazes is intriguing but falls short of being compelling. If organic hazes form, they are likeliest to do s…

2016 The Astrophysical Journal
IUE 82
Data-driven Radiative Hydrodynamic Modeling of the 2014 March 29 X1.0 Solar Flare
DOI: 10.3847/0004-637X/827/1/38 Bibcode: 2016ApJ...827...38R

Liu, Wei; Allred, Joel C.; Kleint, Lucia +2 more

Spectroscopic observations of solar flares provide critical diagnostics of the physical conditions in the flaring atmosphere. Some key features in observed spectra have not yet been accounted for in existing flare models. Here we report a data-driven simulation of the well-observed X1.0 flare on 2014 March 29 that can reconcile some well-known spe…

2016 The Astrophysical Journal
IRIS 82
Suprathermal particle energization in dipolarization fronts: Particle-in-cell simulations
DOI: 10.1002/2016JA022815 Bibcode: 2016JGRA..121.9483L

Angelopoulos, V.; Fu, Huishan; Lu, San

Within dipolarization fronts (DFs) in the Earth's magnetotail, significant magnetic energy is converted to plasma energy, and a significant portion of the electrons and ions therein are accelerated to suprathermal energies. The mechanism that produces these suprathermal particles while simultaneously reducing magnetic field energy is poorly unders…

2016 Journal of Geophysical Research (Space Physics)
Cluster 82
The Characteristics of Solar X-Class Flares and CMEs: A Paradigm for Stellar Superflares and Eruptions?
DOI: 10.1007/s11207-016-0923-0 Bibcode: 2016SoPh..291.1761H

Toriumi, Shin; Guedel, Manuel; Harra, Louise K. +10 more

This paper explores the characteristics of 42 solar X-class flares that were observed between February 2011 and November 2014, with data from the Solar Dynamics Observatory (SDO) and other sources. This flare list includes nine X-class flares that had no associated CMEs. In particular our aim was to determine whether a clear signature could be ide…

2016 Solar Physics
Hinode SOHO 82
SN Refsdal: Photometry and Time Delay Measurements of the First Einstein Cross Supernova
DOI: 10.3847/0004-637X/820/1/50 Bibcode: 2016ApJ...820...50R

Sharon, K.; Molino, A.; Zitrin, A. +16 more

We present the first year of Hubble Space Telescope imaging of the unique supernova (SN) “Refsdal,” a gravitationally lensed SN at z = 1.488 ± 0.001 with multiple images behind the galaxy cluster MACS J1149.6+2223. The first four observed images of SN Refsdal (images S1-S4) exhibited a slow rise (over ∼150 days) to reach a broad peak brightness ar…

2016 The Astrophysical Journal
eHST 82
Infrared Color Selection of Massive Galaxies at z > 3
DOI: 10.3847/0004-637X/816/2/84 Bibcode: 2016ApJ...816...84W

Daddi, E.; Elbaz, D.; Shu, X. +29 more

We introduce a new color selection technique to identify high-redshift, massive galaxies that are systematically missed by Lyman-break selection. The new selection is based on the H160 (H) and Infrared Array Camera (IRAC) 4.5 µm bands, specifically H-[4.5]\gt 2.25 mag. These galaxies, called “HIEROs,” include two major populations…

2016 The Astrophysical Journal
eHST 82
Ionospheric plasma of comet 67P probed by Rosetta at 3 au from the Sun
DOI: 10.1093/mnras/stw2891 Bibcode: 2016MNRAS.462S.331G

Wurz, P.; Altwegg, K.; Glassmeier, K. -H. +23 more

We propose to identify the main sources of ionization of the plasma in the coma of comet 67P/Churyumov-Gerasimenko at different locations in the coma and to quantify their relative importance, for the first time, for close cometocentric distances (<20 km) and large heliocentric distances (>3 au). The ionospheric model proposed is used as an …

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 82
The Age of the Young Bulge-like Population in the Stellar System Terzan 5: Linking the Galactic Bulge to the High-z Universe
DOI: 10.3847/0004-637X/828/2/75 Bibcode: 2016ApJ...828...75F

Dalessandro, E.; Massari, D.; Rich, R. M. +4 more

The Galactic bulge is dominated by an old, metal-rich stellar population. The possible presence and the amount of a young (a few gigayears old) minor component is one of the major issues debated in the literature. Recently, the bulge stellar system Terzan 5 was found to harbor three sub-populations with iron content varying by more than one order …

2016 The Astrophysical Journal
eHST 82
The Distance to M51
DOI: 10.3847/0004-637X/826/1/21 Bibcode: 2016ApJ...826...21M

Dolphin, Andrew E.; Skillman, Evan D.; Berg, Danielle +2 more

Great investments of observing time have been dedicated to the study of nearby spiral galaxies with diverse goals ranging from understanding the star formation process to characterizing their dark matter distributions. Accurate distances are fundamental to interpreting observations of these galaxies, yet many of the best studied nearby galaxies ha…

2016 The Astrophysical Journal
eHST 81
Far-infrared Line Spectra of Active Galaxies from the Herschel/PACS Spectrometer: The Complete Database
DOI: 10.3847/0067-0049/226/2/19 Bibcode: 2016ApJS..226...19F

Spinoglio, Luigi; Fernández-Ontiveros, Juan Antonio; Malkan, Matthew A. +3 more

We present a coherent database of spectroscopic observations of far-IR fine-structure lines from the Herschel/Photoconductor Array Camera and Spectrometer archive for a sample of 170 local active galactic nuclei (AGNs), plus a comparison sample of 20 starburst galaxies and 43 dwarf galaxies. Published Spitzer/IRS and Herschel/SPIRE line fluxes are…

2016 The Astrophysical Journal Supplement Series
Herschel ISO 81