Search Publications

On the Isothermality of Solar Plasmas
DOI: 10.1088/0004-637X/723/1/320 Bibcode: 2010ApJ...723..320L

Klimchuk, J. A.; Landi, E.

Recent measurements have shown that the quiet unstructured solar corona observed at the solar limb is close to isothermal, at a temperature that does not appear to change over wide areas or with time. Some individual active region loop structures have also been found to be nearly isothermal both along their axis and across their cross section. Eve…

2010 The Astrophysical Journal
SOHO 22
Suzaku X-ray Spectra and Pulse Profile Variations During the Superorbital Cycle of LMC X-4
DOI: 10.1088/0004-637X/720/2/1202 Bibcode: 2010ApJ...720.1202H

Vrtilek, Saeqa D.; Hickox, Ryan C.; Hung, Li-Wei +1 more

We present results from spectral and temporal analyses of Suzaku and RXTE observations of the high-mass X-ray binary LMC X-4. Using the full 13 years of available RXTE/all-sky monitor data, we apply the ANOVA and Lomb Normalized Periodogram methods to obtain an improved superorbital period measurement of 30.32 ± 0.04 days. The phase-averaged X-ray…

2010 The Astrophysical Journal
Suzaku 22
Calibration of Hyperspectral Imaging Data: VIRTIS-M Onboard Venus Express
DOI: 10.1109/TGRS.2010.2064325 Bibcode: 2010ITGRS..48.3941C

Drossart, Pierre; Piccioni, Giuseppe; Filacchione, Gianrico +2 more

The Visible and InfraRed Thermal Imaging Spectrometer (VIRTIS) is flying onboard the European Space Agency mission Venus Express and orbiting around Venus since April 11, 2006, providing very valuable remote sensing data of the planet. The instrument combines a double capability: a high-resolution imaging in the visible-infrared range (0.28-5 um) …

2010 IEEE Transactions on Geoscience and Remote Sensing
VenusExpress 22
Latitudinal variations in Titan’s methane and haze from Cassini VIMS observations
DOI: 10.1016/j.icarus.2009.11.003 Bibcode: 2010Icar..206..352P

Sotin, Christophe; Baines, Kevin H.; Buratti, Bonnie J. +9 more

We analyze observations taken with Cassini's Visual and Infrared Mapping Spectrometer (VIMS), to determine the current methane and haze latitudinal distribution between 60°S and 40°N. The methane variation was measured primarily from its absorption band at 0.61 µm, which is optically thin enough to be sensitive to the methane abundance at 20…

2010 Icarus
Cassini 22
Early-type galaxies at large galactocentric radii - I. Stellar kinematics and photometric properties
DOI: 10.1111/j.1365-2966.2010.17282.x Bibcode: 2010MNRAS.408..254S

Forbes, Duncan A.; Couch, Warrick J.; Hau, George K. T. +1 more

We present the results of a combined analysis of the kinematic and photometric properties at large galactocentric radii of a sample of 14 low-luminosity early-type galaxies in the Fornax and Virgo clusters. From Gemini South GMOS long-slit spectroscopic data, we measure radial profiles of the kinematic parameters vrot, σ, h3

2010 Monthly Notices of the Royal Astronomical Society
eHST 22
The clusters Abell 222 and Abell 223: a multi-wavelength view
DOI: 10.1051/0004-6361/201014566 Bibcode: 2010A&A...517A..94D

Bertin, E.; Adami, C.; Durret, F. +1 more

Context. The Abell 222 and 223 clusters are located at an average redshift z ~ 0.21 and are separated by 0.26 deg. Signatures of mergers have been previously found in these clusters, both in X-rays and at optical wavelengths, thus motivating our study. In X-rays, they are relatively bright, and Abell 223 shows a double structure. A filament has al…

2010 Astronomy and Astrophysics
XMM-Newton 22
A strong high altitude narrow jet detected at Saturn's equator
DOI: 10.1029/2010GL045434 Bibcode: 2010GeoRL..3722204G

Hueso, R.; Sánchez-Lavega, A.; García-Melendo, E. +2 more

Here we report the discovery at the upper cloud level of an extremely narrow and strong prograde jet, centered in the middle of the broad equatorial jet. Measurements from images obtained by the Cassini Imaging Science Subsystem (ISS) show that the jet reaches 430 ms-1 ± 16 m s-1 with a peak speed difference of 180 ms-1<…

2010 Geophysical Research Letters
Cassini 22
XMM-Newton RGS observation of the warm absorber in Mrk 279
DOI: 10.1051/0004-6361/201014091 Bibcode: 2010A&A...520A..36E

Kaastra, J. S.; Kriss, G. A.; Arav, N. +5 more

Context. The Seyfert 1 galaxy Mrk 279 was observed by XMM-Newton in November 2005 on three consecutive orbits, showing significant short-scale variability (average soft band variation in flux ~20%). The source is known to host a two-component warm absorber with distinct ionisation states from a previous Chandra observation.
Aims: We study the…

2010 Astronomy and Astrophysics
XMM-Newton 22
Spatially resolved detection of crystallized water ice in a T Tauri object
DOI: 10.1051/0004-6361/200911849 Bibcode: 2010A&A...517A..87S

Wolf, S.; Schegerer, A. A.


Aims: We search for frozen water and its processing around young stellar objects (YSOs of class I/II). We try to detect potential, regional differences in water ice evolution within YSOs, which is relevant to understanding the chemical structure of the progenitors of protoplanetary systems and the evolution of solid materials. Water plays an …

2010 Astronomy and Astrophysics
eHST 22
Differences in solar wind cross-helicity and residual energy during the last two solar minima
DOI: 10.1029/2010GL044570 Bibcode: 2010GeoRL..3717102P

Perri, S.; Balogh, A.

The minimum of solar cycle 23 exhibited anomalous characteristics with respect to its predecessors. Other than the differences in the standard indicators of activity, such as sunspots, polar magnetic fields were also found to be different. These differences had a range of effects in the solar wind. In this work we study the Alfvénicity and the res…

2010 Geophysical Research Letters
Ulysses 22