Search Publications

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
Comet 67P/Churyumov-Gerasimenko preserved the pebbles that formed planetesimals
DOI: 10.1093/mnras/stw2299 Bibcode: 2016MNRAS.462S.132F

Rodriguez, J.; Colangeli, L.; Della Corte, V. +16 more

Solar system formation models predict that the building blocks of planetesimals were mm- to cm-sized pebbles, aggregates of ices and non-volatile materials, consistent with the compact particles ejected by comet 67P/Churyumov-Gerasimenko (67P hereafter) and detected by GIADA (Grain Impact Analyzer and Dust Accumulator) on-board the Rosetta spacecr…

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 93
Jellyfish: the origin and distribution of extreme ram-pressure stripping events in massive galaxy clusters
DOI: 10.1093/mnras/stv2508 Bibcode: 2016MNRAS.455.2994M

Ebeling, Harald; McPartland, Conor; Roediger, Elke +1 more

We investigate the observational signatures and physical origin of ram-pressure stripping (RPS) in 63 massive galaxy clusters at z = 0.3-0.7, based on images obtained with the Hubble Space Telescope. Using a training set of a dozen `jellyfish' galaxies identified earlier in the same imaging data, we define morphological criteria to select 211 addi…

2016 Monthly Notices of the Royal Astronomical Society
eHST 93
A Keck Adaptive Optics Survey of a Representative Sample of Gravitationally Lensed Star-forming Galaxies: High Spatial Resolution Studies of Kinematics and Metallicity Gradients
DOI: 10.3847/0004-637X/820/2/84 Bibcode: 2016ApJ...820...84L

Richard, Johan; Stark, Daniel P.; Ellis, Richard S. +4 more

We discuss spatially resolved emission line spectroscopy secured for a total sample of 15 gravitationally lensed star-forming galaxies at a mean redshift of z≃ 2 based on Keck laser-assisted adaptive optics observations undertaken with the recently improved OSIRIS integral field unit (IFU) spectrograph. By exploiting gravitationally lensed sources…

2016 The Astrophysical Journal
eHST 92
The Bursty Star Formation Histories of Low-mass Galaxies at 0.4 < z < 1 Revealed by Star Formation Rates Measured From Hβ and FUV
DOI: 10.3847/1538-4357/833/1/37 Bibcode: 2016ApJ...833...37G

Barro, Guillermo; Pérez-González, Pablo G.; Bell, Eric F. +17 more

We investigate the burstiness of star formation histories (SFHs) of galaxies at 0.4 < z < 1 by using the ratio of star formation rates (SFRs) measured from Hβ and FUV (1500 Å) (Hβ-to-FUV ratio). Our sample contains 164 galaxies down to stellar mass (M *) of 108.5 M in the CANDELS GOODS-N region, where Team …

2016 The Astrophysical Journal
eHST 92