Search Publications

MOST Observations of Our Nearest Neighbor: Flares on Proxima Centauri
DOI: 10.3847/2041-8205/829/2/L31 Bibcode: 2016ApJ...829L..31D

Davenport, James R. A.; Sasselov, Dimitar; Kipping, David M. +2 more

We present a study of white-light flares from the active M5.5 dwarf Proxima Centauri using the Canadian microsatellite Microvariability and Oscillations of STars. Using 37.6 days of monitoring data from 2014 to 2015, we have detected 66 individual flare events, the largest number of white-light flares observed to date on Proxima Cen. Flare energie…

2016 The Astrophysical Journal
eHST 95
Panchromatic Hubble Andromeda Treasury. XVI. Star Cluster Formation Efficiency and the Clustered Fraction of Young Stars
DOI: 10.3847/0004-637X/827/1/33 Bibcode: 2016ApJ...827...33J

Bell, Eric F.; Dolphin, Andrew E.; Skillman, Evan D. +10 more

We use the Panchromatic Hubble Andromeda Treasury survey data set to perform spatially resolved measurements of star cluster formation efficiency (Γ), the fraction of stellar mass formed in long-lived star clusters. We use robust star formation history and cluster parameter constraints, obtained through color-magnitude diagram analysis of resolved…

2016 The Astrophysical Journal
eHST 95
The evolution of the equivalent width of the Hα emission line and specific star formation rate in star-forming galaxies at 1 < z < 5
DOI: 10.1093/mnras/stw1212 Bibcode: 2016MNRAS.460.3587M

Cullen, F.; McLure, R. J.; Dunlop, J. S. +3 more

We present the results of a study which uses spectral energy distribution (SED) fitting to investigate the evolution of the equivalent width (EW) of the Hα emission line in star-forming galaxies over the redshift interval 1 < z < 5. After first demonstrating the ability of our SED-fitting technique to recover EW(Hα) using a sample of galaxie…

2016 Monthly Notices of the Royal Astronomical Society
eHST 94
X-Ray Detected Active Galactic Nuclei in Dwarf Galaxies at 0 < z < 1
DOI: 10.3847/0004-637X/831/2/203 Bibcode: 2016ApJ...831..203P

Silverman, J. D.; Hickox, R. C.; Greene, J. E. +6 more

We present a sample of accreting supermassive black holes (SMBHs) in dwarf galaxies at z\lt 1. We identify dwarf galaxies in the NEWFIRM Medium Band Survey with stellar masses of {M}\star \lt 3× {10}9 {M} that have spectroscopic redshifts from the DEEP2 survey and lie within the region covered by deep (flux limit…

2016 The Astrophysical Journal
eHST 94
Direct Simulation Monte Carlo modelling of the major species in the coma of comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stw2388 Bibcode: 2016MNRAS.462S.156F

Altwegg, K.; Huang, Z.; Erard, S. +26 more

We analyse the Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) - the Double Focusing Mass Spectrometer data between 2014 August and 2016 February to examine the effect of seasonal variations on the four major species within the coma of 67P/Churyumov-Gerasimenko (H2O, CO2, CO, and O2), resulting f…

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 94
Magnetar-like Activity from the Central Compact Object in the SNR RCW103
DOI: 10.3847/2041-8205/828/1/L13 Bibcode: 2016ApJ...828L..13R

Rea, N.; Esposito, P.; De Luca, A. +4 more

The 6.67 hr periodicity and the variable X-ray flux of the central compact object (CCO) at the center of the supernova remnant RCW 103, named 1E 161348-5055, have been always difficult to interpret within the standard scenarios of an isolated neutron star (NS) or a binary system. On 2016 June 22, the Burst Alert Telescope (BAT) on board Swift dete…

2016 The Astrophysical Journal
XMM-Newton 94
Three-dimensional direct simulation Monte-Carlo modeling of the coma of comet 67P/Churyumov-Gerasimenko observed by the VIRTIS and ROSINA instruments on board Rosetta
DOI: 10.1051/0004-6361/201527889 Bibcode: 2016A&A...588A.134F

Altwegg, K.; Huang, Z.; Erard, S. +26 more

Context. Since its rendezvous with comet 67P/Churyumov-Gerasimenko (67P), the Rosetta spacecraft has provided invaluable information contributing to our understanding of the cometary environment. On board, the VIRTIS and ROSINA instruments can both measure gas parameters in the rarefied cometary atmosphere, the so-called coma, and provide compleme…

2016 Astronomy and Astrophysics
Rosetta 93
Morphology and Molecular Gas Fractions of Local Luminous Infrared Galaxies as a Function of Infrared Luminosity and Merger Stage
DOI: 10.3847/0004-637X/825/2/128 Bibcode: 2016ApJ...825..128L

Sanders, D. B.; Kim, D. -C.; Mirabel, I. F. +8 more

We present a new, detailed analysis of the morphologies and molecular gas fractions (MGFs) for a complete sample of 65 local luminous infrared galaxies from Great Observatories All-Sky Luminous Infrared Galaxies (LIRG) Survey using high resolution I-band images from The Hubble Space Telescope, the University of Hawaii 2.2 m Telescope and the Pan-S…

2016 The Astrophysical Journal
eHST 93
Simulations of the Mg II k and Ca II 8542 lines from an Alfvén Wave-heated Flare Chromosphere
DOI: 10.3847/0004-637X/827/2/101 Bibcode: 2016ApJ...827..101K

Kerr, Graham S.; Fletcher, Lyndsay.; Russell, Alexander J. B. +1 more

We use radiation hydrodynamic simulations to examine two models of solar flare chromospheric heating: Alfvén wave dissipation and electron beam collisional losses. Both mechanisms are capable of strong chromospheric heating, and we show that the distinctive atmospheric evolution in the mid-to-upper chromosphere results in Mg II k-line emission tha…

2016 The Astrophysical Journal
IRIS 93
Global Sausage Oscillation of Solar Flare Loops Detected by the Interface Region Imaging Spectrograph
DOI: 10.3847/2041-8205/823/1/L16 Bibcode: 2016ApJ...823L..16T

Reeves, Katharine K.; Chen, Bin; He, Jiansen +4 more

An observation from the Interface Region Imaging Spectrograph reveals coherent oscillations in the loops of an M1.6 flare on 2015 March 12. Both the intensity and Doppler shift of Fe xxi 1354.08 Å show clear oscillations with a period of ∼25 s. Remarkably similar oscillations were also detected in the soft X-ray flux recorded by the Geostationary …

2016 The Astrophysical Journal
Hinode IRIS 93