Search Publications

Saturn's magnetospheric interaction with Titan as defined by Cassini encounters T9 and T18: New results
DOI: 10.1016/j.pss.2009.09.017 Bibcode: 2010P&SS...58..327S

Coates, A. J.; Johnson, R. E.; Wahlund, J. -E. +8 more

We present new results of Cassini's T9 flyby with complementary observations from T18. Based on Cassini plasma spectrometer (CAPS) and Cassini magnetometer (MAG), compositional evidence shows the upstream flow for both T9 and T18 appears composed of light ions (H + and H 2+), with external pressures ∼30 times lower…

2010 Planetary and Space Science
Cassini 38
Erratum: "Determining Titan's Spin State from Cassini Radar Images"
DOI: 10.1088/0004-6256/139/1/311 Bibcode: 2010AJ....139..311S

Iess, Luciano; Cassini RADAR Team; Stiles, Bryan W. +12 more

We previously reported an initial determination of Titan's rotational state from fits to overlapping radar images. We have since discovered a coding error in software used to make these fits, which led to systematic offsets of 1-2 km in recovered positions. While our principal results remain qualitatively unchanged, with this error corrected, the …

2010 The Astronomical Journal
Cassini 38
Pre-main-sequence Turn-On as a Chronometer for Young Clusters: NGC 346 as a Benchmark
DOI: 10.1088/2041-8205/712/1/L63 Bibcode: 2010ApJ...712L..63C

Prada Moroni, P. G.; Degl'Innocenti, S.; Cignoni, M. +4 more

We present a novel approach to deriving the age of very young star clusters, by using the Turn-On (TOn). The TOn is the point in the color-magnitude diagram (CMD) where the pre-main sequence (PMS) joins the main sequence (MS). In the MS luminosity function (LF) of the cluster, the TOn is identified as a peak followed by a dip. We propose that by c…

2010 The Astrophysical Journal
eHST 38
Star formation in the outer filaments of NGC 1275
DOI: 10.1111/j.1365-2966.2010.16474.x Bibcode: 2010MNRAS.405..115C

Fabian, A. C.; Gallagher, J. S.; Conselice, C. J. +5 more

We present photometry of the outer star clusters in NGC 1275, the brightest galaxy in the Perseus cluster. The observations were taken using the Hubble Space Telescope Advanced Camera for Surveys. We focus on two stellar regions in the south and south-east, far from the nucleus of the low-velocity system (~22kpc). These regions of extended star fo…

2010 Monthly Notices of the Royal Astronomical Society
eHST 38
Evolution of low-altitude and ring current ENA emissions from a moderate magnetospheric storm: Continuous and simultaneous TWINS observations
DOI: 10.1029/2010JA015429 Bibcode: 2010JGRA..11511209V

Roelof, E.; McComas, D. J.; Brandt, P. C. +6 more

The moderate storm of 22 July 2009 is the largest measured during the extended solar minimum between December 2006 and March 2010. We present observations of this storm made by the two wide-angle imaging neutral-atom spectrometers (TWINS) mission. The TWINS mission measures energetic neutral atoms (ENAs) using sensors mounted on two separate space…

2010 Journal of Geophysical Research (Space Physics)
Cassini 38
Jupiter After the 2009 Impact: Hubble Space Telescope Imaging of the Impact-generated Debris and its Temporal Evolution
DOI: 10.1088/2041-8205/715/2/L150 Bibcode: 2010ApJ...715L.150H

Hueso, R.; Sánchez-Lavega, A.; Fletcher, L. N. +9 more

We report Hubble Space Telescope images of Jupiter during the aftermath of an impact by an unknown object in 2009 July. The 2009 impact-created debris field evolved more slowly than those created in 1994 by the collision of the tidally disrupted comet D/Shoemaker-Levy 9 (SL9). The slower evolution, in conjunction with the isolated nature of this s…

2010 The Astrophysical Journal
eHST 38
Estimation of the escape of photoelectrons from Mars in 2004 liberated by the ionization of carbon dioxide and atomic oxygen
DOI: 10.1016/j.icarus.2009.03.024 Bibcode: 2010Icar..206...50F

Coates, A. J.; Fedorov, A.; Barabash, S. +8 more

Photoelectron peaks in the atmosphere of Mars caused by the ionization of carbon dioxide and atomic oxygen by solar 30.4 nm photons have been observed by the Electron Spectrometer (ELS), a component of the Mars Express (MEx) Analyzer of Space Plasmas and Energetic Atoms (ASPERA-3) experiment. Ionization mostly occurs at the Mars exobase with the m…

2010 Icarus
MEx 38
Fine-structure infrared lines from the Cassiopeia A knots
DOI: 10.1051/0004-6361/200810366 Bibcode: 2010A&A...509A..59D

Sunyaev, R. A.; Docenko, D.


Aims: Archival observations of infrared fine-structure lines of the young Galactic supernova remnant Cassiopeia A allow us to test existing models and determine the physical parameters of various regions of the fast-moving knots, which are metal-dominated clouds of material ejected by the supernova explosion.
Methods: The fluxes of far-i…

2010 Astronomy and Astrophysics
ISO eHST 38
First detection of the methylidyne cation (CH+) fundamental rotational line with the Herschel/SPIRE FTS
DOI: 10.1051/0004-6361/201014656 Bibcode: 2010A&A...518L.117N

Miville-Deschênes, M. -A.; Boulanger, F.; Abergel, A. +42 more


Aims: To follow the species chemistry arising in diverse sources of the Galaxy with Herschel.
Methods: SPIRE FTS sparse sampled maps of the Orion bar & compact HII regions G29.96-0.02 and G32.80+0.19 have been analyzed.
Results: Beyond the wealth of atomic and molecular lines detected in the high-resolution spectra obtained with…

2010 Astronomy and Astrophysics
Herschel 38
A Late Amazonian alteration layer related to local volcanism on Mars
DOI: 10.1016/j.icarus.2009.10.015 Bibcode: 2010Icar..207..265M

Mangold, N.; Le Mouélic, S.; Mustard, J. F. +7 more

Hydrated minerals on Mars are most commonly found in ancient terrains dating to the first billion years of the planet's evolution. Here we discuss the identification of a hydrated light-toned rock unit present in one Chasma of the Noctis Labyrinthus region. Stratigraphy and topography show that this alteration layer is part of a thin unit that dra…

2010 Icarus
MEx 38