Search Publications

Clouds on the Hot Jupiter HD189733b: Constraints from the Reflection Spectrum
DOI: 10.1088/0004-637X/786/2/154 Bibcode: 2014ApJ...786..154B

Aigrain, S.; Fletcher, L. N.; Irwin, P. G. J. +4 more

The hot Jupiter HD 189733b is probably the best studied of the known extrasolar planets, with published transit and eclipse spectra covering the near UV to mid-IR range. Recent work on the transmission spectrum has shown clear evidence for the presence of clouds in its atmosphere, which significantly increases the model atmosphere parameter space …

2014 The Astrophysical Journal
eHST 57
New Detections of Arsenic, Selenium, and Other Heavy Elements in Two Metal-poor Stars
DOI: 10.1088/0004-637X/791/1/32 Bibcode: 2014ApJ...791...32R

Beers, Timothy C.; Roederer, Ian U.; Frebel, Anna +6 more

We use the Space Telescope Imaging Spectrograph on board the Hubble Space Telescope to obtain new high-quality spectra covering the 1900 <=λ <= 2360 Å wavelength range for two metal-poor stars, HD 108317 and HD 128279. We derive abundances of Cu II, Zn II, As I, Se I, Mo II, and Cd II, which have not been detected previously in either star. …

2014 The Astrophysical Journal
eHST 57
Long-period intensity pulsations in the solar corona during activity cycle 23
DOI: 10.1051/0004-6361/201322572 Bibcode: 2014A&A...563A...8A

Auchère, F.; Bocchialini, K.; Solomon, J. +1 more

We report on the detection (10σ) of 917 events of long-period (3 to 16 h) intensity pulsations in the 19.5 nm passband of the SOHO Extreme ultraviolet Imaging Telescope. The data set spans from January 1997 to July 2010, i.e. the entire solar cycle 23 and the beginning of cycle 24. The events can last for up to six days and have relative amplitude…

2014 Astronomy and Astrophysics
SOHO 57
"TNOs are Cool": A survey of the trans-Neptunian region. XI. A Herschel-PACS view of 16 Centaurs
DOI: 10.1051/0004-6361/201322377 Bibcode: 2014A&A...564A..92D

Fornasier, S.; Lellouch, E.; Kiss, C. +13 more

Context. Centaurs are the transitional population between trans-Neptunian objects (TNOs) and Jupiter-family comets. Their physical properties provide an insight into TNO properties, but only under restricted conditions since Centaurs are closer to the Sun and Earth. For this reason it is possible to access the smaller ones, which is more difficult…

2014 Astronomy and Astrophysics
Herschel 56
The many sides of RCW 86: a Type Ia supernova remnant evolving in its progenitor's wind bubble
DOI: 10.1093/mnras/stu667 Bibcode: 2014MNRAS.441.3040B

Vink, Jacco; Bamba, Aya; Chiotellis, Alexandros +1 more

We present the results of a detailed investigation of the Galactic supernova remnant RCW 86 using the XMM-Newton X-ray telescope. RCW 86 is the probable remnant of SN 185 A.D., a supernova that likely exploded inside a wind-blown cavity. We use the XMM-Newton Reflection Grating Spectrometer to derive precise temperatures and ionization ages of the…

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 56
An independent determination of Fomalhaut b's orbit and the dynamical effects on the outer dust belt
DOI: 10.1051/0004-6361/201322229 Bibcode: 2014A&A...561A..43B

Augereau, J. -C.; Ertel, S.; Lebreton, J. +7 more

Context. The nearby star Fomalhaut harbors a cold, moderately eccentric (e ~ 0.1) dust belt with a sharp inner edge near 133 au. A low-mass, common proper motion companion, Fomalhaut b (Fom b), was discovered near the inner edge and was identified as a planet candidate that could account for the belt morphology. However, the most recent orbit dete…

2014 Astronomy and Astrophysics
eHST 56
The Corona of HD 189733 and its X-Ray Activity
DOI: 10.1088/0004-637X/785/2/145 Bibcode: 2014ApJ...785..145P

Günther, H. M.; Sciortino, S.; Drake, J. J. +5 more

Testing whether close-in massive exoplanets (hot Jupiters) can enhance the stellar activity in their host primary is crucial for the models of stellar and planetary evolution. Among systems with hot Jupiters, HD 189733 is one of the best studied because of its proximity, strong activity, and the presence of a transiting planet, which allows transm…

2014 The Astrophysical Journal
XMM-Newton 56
Herschel-ATLAS: modelling the first strong gravitational lenses
DOI: 10.1093/mnras/stu305 Bibcode: 2014MNRAS.440.2013D

Ivison, R. J.; Smith, M.; Cooray, A. +14 more

We have determined the mass density radial profiles of the first five strong gravitational lens systems discovered by the Herschel Astrophysical Terahertz Large Area Survey. We present an enhancement of the semilinear lens inversion method of Warren & Dye which allows simultaneous reconstruction of several different wavebands and apply this to…

2014 Monthly Notices of the Royal Astronomical Society
eHST 56
Three New Cool Brown Dwarfs Discovered with the Wide-field Infrared Survey Explorer (WISE) and an Improved Spectrum of the Y0 Dwarf WISE J041022.71+150248.4
DOI: 10.1088/0004-6256/147/5/113 Bibcode: 2014AJ....147..113C

Gould, Andrew; Cushing, Michael C.; Kirkpatrick, J. Davy +3 more

As part of a larger search of Wide-field Infrared Survey Explorer (WISE) data for cool brown dwarfs with effective temperatures less than 1000 K, we present the discovery of three new cool brown dwarfs with spectral types later than T7. Using low-resolution, near-infrared spectra obtained with the NASA Infrared Telescope Facility and the Hubble Sp…

2014 The Astronomical Journal
eHST 56
Water in star-forming regions with Herschel (WISH). V. The physical conditions in low-mass protostellar outflows revealed by multi-transition water observations
DOI: 10.1051/0004-6361/201424267 Bibcode: 2014A&A...572A..21M

Liseau, R.; van Dishoeck, E. F.; Bergin, E. A. +17 more

Context. Outflows are an important part of the star formation process as both the result of ongoing active accretion and one of the main sources of mechanical feedback on small scales. Water is the ideal tracer of these effects because it is present in high abundance for the conditions expected in various parts of the protostar, particularly the o…

2014 Astronomy and Astrophysics
Herschel 56