Search Publications

Time variability and heterogeneity in the coma of 67P/Churyumov-Gerasimenko
DOI: 10.1126/science.aaa0276 Bibcode: 2015Sci...347a0276H

Wurz, P.; Bochsler, P.; Altwegg, K. +33 more

Comets contain the best-preserved material from the beginning of our planetary system. Their nuclei and comae composition reveal clues about physical and chemical conditions during the early solar system when comets formed. ROSINA (Rosetta Orbiter Spectrometer for Ion and Neutral Analysis) onboard the Rosetta spacecraft has measured the coma compo…

2015 Science
Rosetta 123
Resonant Absorption of Transverse Oscillations and Associated Heating in a Solar Prominence. II. Numerical Aspects
DOI: 10.1088/0004-637X/809/1/72 Bibcode: 2015ApJ...809...72A

De Pontieu, B.; Yokoyama, T.; Okamoto, T. J. +3 more

Transverse magnetohydrodynamic (MHD) waves are ubiquitous in the solar atmosphere and may be responsible for generating the Sun’s million-degree outer atmosphere. However, direct evidence of the dissipation process and heating from these waves remains elusive. Through advanced numerical simulations combined with appropriate forward modeling of a p…

2015 The Astrophysical Journal
Hinode IRIS 122
Global Trends of CME Deflections Based on CME and Solar Parameters
DOI: 10.1088/0004-637X/805/2/168 Bibcode: 2015ApJ...805..168K

Kay, C.; Opher, M.; Evans, R. M.

Accurate space weather forecasting requires knowledge of the trajectory of coronal mass ejections (CMEs), including any deflections close to the Sun or through interplanetary space. Kay et al. introduced ForeCAT, a model of CME deflection resulting from the background solar magnetic field. For a magnetic field solution corresponding to Carrington …

2015 The Astrophysical Journal
SOHO 122
The Lyman Alpha Reference Sample. V. The Impact of Neutral ISM Kinematics and Geometry on Lyα Escape
DOI: 10.1088/0004-637X/805/1/14 Bibcode: 2015ApJ...805...14R

Verhamme, Anne; Cannon, John M.; Hayes, Matthew +15 more

We present high-resolution far-UV spectroscopy of the 14 galaxies of the Lyα Reference Sample; a sample of strongly star-forming galaxies at low redshifts (0.028 < z < 0.18). We compare the derived properties to global properties derived from multi-band imaging and 21 cm H i interferometry and single-dish observations, as well as archival op…

2015 The Astrophysical Journal
eHST 121
Detection of Broad Hα Emission Lines in the Late-time Spectra of a Hydrogen-poor Superluminous Supernova
DOI: 10.1088/0004-637X/814/2/108 Bibcode: 2015ApJ...814..108Y

Cenko, S. B.; Gal-Yam, A.; Kulkarni, S. R. +14 more

iPTF13ehe is a hydrogen-poor superluminous supernova (SLSN) at z = 0.3434, with a slow-evolving light curve and spectral features similar to SN2007bi. It rises in 83-148 days to reach a peak bolometric luminosity of ∼1.3 × 1044 erg s-1, then decays slowly at 0.015 mag day-1. The measured ejecta velocity is ∼ 13,000…

2015 The Astrophysical Journal
eHST 121
Leo P: An Unquenched Very Low-mass Galaxy
DOI: 10.1088/0004-637X/812/2/158 Bibcode: 2015ApJ...812..158M

McQuinn, Kristen B. W.; Cannon, John M.; Skillman, Evan D. +8 more

Leo P is a low-luminosity dwarf galaxy discovered through the blind H i Arecibo Legacy Fast ALFA survey. The H i and follow-up optical observations have shown that Leo P is a gas-rich dwarf galaxy with active star formation, an underlying older population, and an extremely low oxygen abundance. We have obtained optical imaging with the Hubble Spac…

2015 The Astrophysical Journal
eHST 121
Inflation physics from the cosmic microwave background and large scale structure
DOI: 10.1016/j.astropartphys.2014.05.013 Bibcode: 2015APh....63...55A

Hu, W.; Bond, J. R.; Borrill, J. +91 more

Fluctuations in the intensity and polarization of the cosmic microwave background (CMB) and the large-scale distribution of matter in the universe each contain clues about the nature of the earliest moments of time. The next generation of CMB and large-scale structure (LSS) experiments are poised to test the leading paradigm for these earliest mom…

2015 Astroparticle Physics
Planck 120
Stellar Populations from Spectroscopy of a Large Sample of Quiescent Galaxies at Z > 1: Measuring the Contribution of Progenitor Bias to Early Size Growth
DOI: 10.1088/0004-637X/799/2/206 Bibcode: 2015ApJ...799..206B

Ellis, Richard S.; Belli, Sirio; Newman, Andrew B.

We analyze the stellar populations of a sample of 62 massive (log M */M > 10.7) galaxies in the redshift range 1 < z < 1.6, with the main goal of investigating the role of recent quenching in the size growth of quiescent galaxies. We demonstrate that our sample is not biased toward bright, compact, or young galaxie…

2015 The Astrophysical Journal
eHST 120
Revealing the complex nature of the strong gravitationally lensed system H-ATLAS J090311.6+003906 using ALMA
DOI: 10.1093/mnras/stv1442 Bibcode: 2015MNRAS.452.2258D

Ivison, R. J.; Smail, Ian; Cooray, A. +13 more

We have modelled Atacama Large Millimetre/sub-millimetre Array (ALMA) long baseline imaging of the strong gravitational lens system H-ATLAS J090311.6+003906 (SDP.81). We have reconstructed the distribution of band 6 and 7 continuum emission in the z = 3.042 source and determined its kinematic properties by reconstructing CO(5-4) and CO(8-7) line e…

2015 Monthly Notices of the Royal Astronomical Society
eHST 120
Self-consistent two-phase AGN torus models⋆. SED library for observers
DOI: 10.1051/0004-6361/201526034 Bibcode: 2015A&A...583A.120S

Siebenmorgen, Ralf; Efstathiou, Andreas; Heymann, Frank

We assume that dust near active galactic nuclei (AGNs) is distributed in a torus-like geometry, which can be described as a clumpy medium or a homogeneous disk, or as a combination of the two (i.e. a two-phase medium). The dust particles considered are fluffy and have higher submillimeter emissivities than grains in the diffuse interstellar medium…

2015 Astronomy and Astrophysics
Herschel 119