Search Publications

The primordial nucleus of comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201526968 Bibcode: 2016A&A...592A..63D

Jorda, L.; Lamy, P. L.; Lara, L. M. +45 more

Context. We investigate the formation and evolution of comet nuclei and other trans-Neptunian objects (TNOs) in the solar nebula and primordial disk prior to the giant planet orbit instability foreseen by the Nice model.
Aims: Our goal is to determine whether most observed comet nuclei are primordial rubble-pile survivors that formed in the s…

2016 Astronomy and Astrophysics
Rosetta 158
Q1549-C25: A Clean Source of Lyman-Continuum Emission at z = 3.15
DOI: 10.3847/2041-8205/826/2/L24 Bibcode: 2016ApJ...826L..24S

Siana, Brian; Shapley, Alice E.; Steidel, Charles C. +5 more

We present observations of Q1549-C25, an ∼ {L}* star-forming galaxy at z = 3.15 for which Lyman-continuum (LyC) radiation is significantly detected in deep Keck/LRIS spectroscopy. We find no evidence of contamination from a lower-redshift interloper close to the line of sight in the high signal-to-noise spectrum of Q1549-C25. Furthermo…

2016 The Astrophysical Journal
eHST 157
A radio-pulsing white dwarf binary star
DOI: 10.1038/nature18620 Bibcode: 2016Natur.537..374M

Gänsicke, B. T.; Dhillon, V. S.; Pala, A. F. +23 more

White dwarfs are compact stars, similar in size to Earth but approximately 200,000 times more massive. Isolated white dwarfs emit most of their power from ultraviolet to near-infrared wavelengths, but when in close orbits with less dense stars, white dwarfs can strip material from their companions and the resulting mass transfer can generate atomi…

2016 Nature
Herschel eHST 157
Refractory and semi-volatile organics at the surface of comet 67P/Churyumov-Gerasimenko: Insights from the VIRTIS/Rosetta imaging spectrometer
DOI: 10.1016/j.icarus.2016.02.028 Bibcode: 2016Icar..272...32Q

Fornasier, S.; Erard, S.; Drossart, P. +34 more

The VIRTIS (Visible, Infrared and Thermal Imaging Spectrometer) instrument aboard the Rosetta spacecraft has performed extensive spectral mapping of the surface of comet 67P/Churyumov-Gerasimenko in the range 0.3-5 µm. The reflectance spectra collected across the surface display a low reflectance factor over the whole spectral range, two spe…

2016 Icarus
Rosetta 157
The Coupled Physical Structure of Gas and Dust in the IM Lup Protoplanetary Disk
DOI: 10.3847/0004-637X/832/2/110 Bibcode: 2016ApJ...832..110C

Wilner, David J.; Cleeves, L. Ilsedore; Andrews, Sean M. +4 more

The spatial distribution of gas and solids in protoplanetary disks determines the composition and formation efficiency of planetary systems. A number of disks show starkly different distributions for the gas and small grains compared to millimeter-centimeter-sized dust. We present new Atacama Large Millimeter/Submillimeter Array observations of th…

2016 The Astrophysical Journal
Gaia 156
The faint radio sky: radio astronomy becomes mainstream
DOI: 10.1007/s00159-016-0098-6 Bibcode: 2016A&ARv..24...13P

Padovani, Paolo

Radio astronomy has changed. For years it studied relatively rare sources, which emit mostly non-thermal radiation across the entire electromagnetic spectrum, I.e. radio quasars and radio galaxies. Now, it is reaching such faint flux densities that it detects mainly star-forming galaxies and the more common radio-quiet active galactic nuclei. Thes…

2016 Astronomy and Astrophysics Review
eHST 155
Beyond 31 mag arcsec-2: The Frontier of Low Surface Brightness Imaging with the Largest Optical Telescopes
DOI: 10.3847/0004-637X/823/2/123 Bibcode: 2016ApJ...823..123T

Trujillo, Ignacio; Fliri, Jüergen

The detection of structures in the sky with optical surface brightnesses fainter than 30 mag arcsec-2 (3σ in 10 × 10 arcsec boxes; r-band) has remained elusive in current photometric deep surveys. Here we show how present-day telescopes of 10 m class can provide broadband imaging 1.5-2 mag deeper than most previous results within a reas…

2016 The Astrophysical Journal
Planck 154
Aggregate dust particles at comet 67P/Churyumov-Gerasimenko
DOI: 10.1038/nature19091 Bibcode: 2016Natur.537...73B

Jessberger, Elmar K.; Torkar, Klaus; Levasseur-Regourd, Anny-Chantal +9 more

Comets are thought to preserve almost pristine dust particles, thus providing a unique sample of the properties of the early solar nebula. The microscopic properties of this dust played a key part in particle aggregation during the formation of the Solar System. Cometary dust was previously considered to comprise irregular, fluffy agglomerates on …

2016 Nature
Rosetta 154
The Atmospheric Circulation of a Nine-hot-Jupiter Sample: Probing Circulation and Chemistry over a Wide Phase Space
DOI: 10.3847/0004-637X/821/1/9 Bibcode: 2016ApJ...821....9K

Fortney, Jonathan J.; Sing, David K.; Kataria, Tiffany +4 more

We present results from an atmospheric circulation study of nine hot Jupiters that compose a large transmission spectral survey using the Hubble and Spitzer Space Telescopes. These observations exhibit a range of spectral behavior over optical and infrared wavelengths, suggesting diverse cloud and haze properties in their atmospheres. By utilizing…

2016 The Astrophysical Journal
eHST 153
Magnetohydrodynamic simulation of interplanetary propagation of multiple coronal mass ejections with internal magnetic flux rope (SUSANOO-CME)
DOI: 10.1002/2015SW001308 Bibcode: 2016SpWea..14...56S

Kataoka, R.; Shiota, D.

Coronal mass ejections (CMEs) are the most important drivers of various types of space weather disturbance. Here we report a newly developed magnetohydrodynamic (MHD) simulation of the solar wind, including a series of multiple CMEs with internal spheromak-type magnetic fields. First, the polarity of the spheromak magnetic field is set as determin…

2016 Space Weather
SOHO 153