Search Publications

From Voyager-IRIS to Cassini-CIRS: Interannual variability in Saturn’s stratosphere?
DOI: 10.1016/j.icarus.2014.02.009 Bibcode: 2014Icar..233..281S

Fletcher, L. N.; Irwin, P. G. J.; Sinclair, J. A. +4 more

We present an intercomparison of Saturn’s stratosphere between Voyager 1-IRIS observations in 1980 and Cassini-CIRS observations in 2009 and 2010. Over a saturnian year (∼29.5 years) has now passed since the Voyager flybys of Saturn in 1980/1981. Cassini observations in 2009/2010 capture Saturn in the same season as Voyager observations (just afte…

2014 Icarus
Cassini 19
Far-infrared Extinction Mapping of Infrared Dark Clouds
DOI: 10.1088/2041-8205/780/2/L29 Bibcode: 2014ApJ...780L..29L

Tan, Jonathan C.; Lim, Wanggi

Progress in understanding star formation requires detailed observational constraints on the initial conditions, i.e., dense clumps and cores in giant molecular clouds that are on the verge of gravitational instability. Such structures have been studied by their extinction of near-infrared and, more recently, mid-infrared (MIR) background light. It…

2014 The Astrophysical Journal
Herschel 19
The white dwarf cooling sequence of 47 Tucanae
DOI: 10.1051/0004-6361/201424652 Bibcode: 2014A&A...571A..56G

Althaus, Leandro G.; Torres, Santiago; Miller Bertolami, Marcelo M. +1 more

Context. 47 Tucanae is one of the most interesting, well-observed, and theoretically studied globular clusters. This allows us to determine the reliability of our understanding of white dwarf cooling sequences, to compare different methods of determining its age, and to assess other important characteristics, such as its star formation history.

2014 Astronomy and Astrophysics
eHST 19
GS-TEC: the Gaia spectrophotometry transient events classifier
DOI: 10.1093/mnras/stu837 Bibcode: 2014MNRAS.442..327B

Wyrzykowski, Łukasz; Blagorodnova, Nadejda; Irwin, Mike +2 more

We present an algorithm for classifying the nearby transient objects detected by the Gaia satellite. The algorithm will use the low-resolution spectra from the blue and red spectrophotometers on board the satellite. Taking a Bayesian approach, we model the spectra using the newly constructed reference spectral library and literature-driven priors.…

2014 Monthly Notices of the Royal Astronomical Society
Gaia 19
Pulse phase-coherent timing and spectroscopy of CXOU J164710.2-45521 outbursts
DOI: 10.1093/mnras/stu603 Bibcode: 2014MNRAS.441.1305R

Esposito, Paolo; Turolla, Roberto; Rea, Nanda +5 more

We present a long-term phase-coherent timing analysis and pulse-phase resolved spectroscopy for the two outbursts observed from the transient anomalous X-ray pulsar CXOU J164710.2-455216. For the first outburst we used 11 Chandra and XMM-Newton observations between 2006 September and 2009 August, the longest baseline yet for this source. We obtain…

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 19
No More Active Galactic Nuclei in Clumpy Disks Than in Smooth Galaxies at z ~ 2 in CANDELS/3D-HST
DOI: 10.1088/0004-637X/793/2/101 Bibcode: 2014ApJ...793..101T

Barro, Guillermo; Bell, Eric F.; Ferguson, Henry C. +23 more

We use CANDELS imaging, 3D-HST spectroscopy, and Chandra X-ray data to investigate if active galactic nuclei (AGNs) are preferentially fueled by violent disk instabilities funneling gas into galaxy centers at 1.3 < z < 2.4. We select galaxies undergoing gravitational instabilities using the number of clumps and degree of patchiness as proxie…

2014 The Astrophysical Journal
eHST 19
Characterizing the Structure of Diffuse Emission in Hi-GAL Maps
DOI: 10.1088/0004-637X/788/1/3 Bibcode: 2014ApJ...788....3E

Natoli, P.; Paladini, R.; Rygl, K. L. J. +18 more

We present a study of the structure of the Galactic interstellar medium (ISM) through the Δ-variance technique, related to the power spectrum and the fractal properties of infrared/submillimeter maps. Through this method, it is possible to provide quantitative parameters, which are useful for characterizing different morphological and physical con…

2014 The Astrophysical Journal
Herschel 19
Formation and Decay of Rudimentary Penumbra around a Pore
DOI: 10.1088/0004-637X/796/2/77 Bibcode: 2014ApJ...796...77W

Kitai, Reizaburo; Otsuji, Kenichi; Watanabe, Hiroko

We analyze the evolution of a pore in the active region NOAA 10940 using the data obtained by the Hinode satellite on 2007 February 3. The pore we analyzed showed the formation of a rudimentary penumbra structure, succeeded by an abrupt disappearance after about 5 hr. The pore had an approximate radius of 3.5 Mm and a total magnetic flux of 3.0 × …

2014 The Astrophysical Journal
Hinode 19
Cassini ISS mutual event astrometry of the mid-sized Saturnian satellites 2005-2012
DOI: 10.1051/0004-6361/201424555 Bibcode: 2014A&A...572A..43C

Cooper, N. J.; Lainey, V.; Murray, C. D. +3 more


Aims: We present astrometric observations of the Saturnian satellites Mimas, Enceladus, Tethys, Dione, and Rhea from Cassini Imaging Science Subsystem (ISS) narrow-angle camera (NAC) images. Image sequences were designed to observe mutual occultations between these satellites.
Methods: The positions of satellite centres were estimated by…

2014 Astronomy and Astrophysics
Cassini 19
Discovery of Enhanced Radiative Recombination Continua of He-like Iron and Calcium from IC 443 and its Implications
DOI: 10.1088/0004-637X/784/1/74 Bibcode: 2014ApJ...784...74O

Koyama, Katsuji; Uchida, Hiroyuki; Tsuru, Takeshi Go +3 more

We present deep observations of the Galactic supernova remnant IC 443 with the Suzaku X-ray satellite. We find prominent K-shell lines from iron and nickel, together with a triangle residual at 8-10 keV, which corresponds to the energy of the radiative recombination continuum (RRC) of He-like iron. In addition, the wavy residuals have been seen at…

2014 The Astrophysical Journal
Suzaku 19