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Craters, smooth terrains, flows, and layering on the comet nuclei
DOI: 10.1134/S0038094607020037 Bibcode: 2007SoSyR..41..109B

Keller, H. U.; Basilevsky, A. T.

The paper considers morphology of craters, smooth surfaces, and flows as well as signatures of layering observed on nuclei of Borrelly, Wild 2, and Tempel 1. In our analysis, we emphasize the role of the so-called planation process, which involves avalanche-type flows and can be responsible for the formation of flow-like features, smooth terrains,…

2007 Solar System Research
Rosetta 26
Structure through colour: a pixel approach towards understanding galaxies
DOI: 10.1111/j.1365-2966.2007.12132.x Bibcode: 2007MNRAS.380..571L

Conselice, C. J.; Lanyon-Foster, M. M.; Merrifield, M. R.

We present a study of pixel colour-magnitude diagrams (pCMDs) for a sample of 69 nearby galaxies chosen to span a wide range of Hubble types. Our goal is to determine how useful a pixel approach is for studying galaxies according to their stellar light distributions and content. The galaxy images were analysed on a pixel-by-pixel basis to reveal t…

2007 Monthly Notices of the Royal Astronomical Society
eHST 26
Numerical modeling of the magnetic topology near Mars auroral observations
DOI: 10.1029/2007GL031806 Bibcode: 2007GeoRL..3424202L

Barabash, S.; Lundin, R.; Winningham, J. D. +6 more

Magnetohydrodynamic (MHD) simulations of the Mars magnetic field topology are presented for the auroral observations reported from the Mars Express SPICAM instrument. It is found that the field lines closest to the assumed emission location are open. That is, they are connected to the interplanetary magnetic field, thus allowing access for solar w…

2007 Geophysical Research Letters
MEx 26
The Globular Cluster System in NGC 5866: Optical Observations from Hubble Space Telescope Advanced Camera for Surveys
DOI: 10.1086/521218 Bibcode: 2007ApJ...668..209C

Blakeslee, John P.; Cantiello, Michele; Raimondo, Gabriella

We perform a detailed study of the globular cluster (GC) system in the galaxy NGC 5866 based on F435W, F555W, and F625W (~B, V, and R) Hubble Space Telescope Advanced Camera for Surveys images. Adopting color, size, and shape selection criteria, the final list of GC candidates comprises 109 objects, with small estimated contamination from backgrou…

2007 The Astrophysical Journal
eHST 26
Evidence for the Importance of Resonance Scattering in X-Ray Emission Line Profiles of the O Star ζ Puppis
DOI: 10.1086/512031 Bibcode: 2007ApJ...659..642L

Leutenegger, Maurice A.; Kahn, Steven M.; Owocki, Stanley P. +1 more

We fit the Doppler profiles of the He-like triplet complexes of O VII and N VI in the X-ray spectrum of the O star ζ Pup, using XMM-Newton RGS data collected over ~400 ks of exposure. We find that they cannot be well fit if the resonance and intercombination lines are constrained to have the same profile shape. However, a significantly better fit …

2007 The Astrophysical Journal
XMM-Newton 26
PAHs in the halo of NGC 5529
DOI: 10.1051/0004-6361:20077729 Bibcode: 2007A&A...474..461I

Madden, S.; Parkin, T.; Irwin, J. A. +1 more

We present sensitive ISO λ 6.7~µm observations of the edge-on galaxy, NGC 5529, finding an extensive MIR halo around NGC 5529. The emission is dominated by PAHs in this band. The PAH halo has an exponential scale height of 3.7 kpc but can still be detected as far as ≈10 kpc from the plane to the limits of the high dynamic range (1770/1) data…

2007 Astronomy and Astrophysics
ISO 26
Direct imaging of the young spectroscopic binary HD 160934
DOI: 10.1051/0004-6361:20066765 Bibcode: 2007A&A...463..707H

Henning, T.; Brandner, W.; Hormuth, F. +2 more

Context: Members of nearby moving groups are promising candidates for the detection of stellar or substellar companions by direct imaging. Mass estimates and magnitude measurements of detected companions to young stars are valuable input data to facilitate the refinement of existing pre-main-sequence stellar models. In this paper we report on our …

2007 Astronomy and Astrophysics
eHST 26
The Stellar Content of the COSMOS Field as Derived from Morphological and SED-based Star/Galaxy Separation
DOI: 10.1086/516600 Bibcode: 2007ApJS..172..545R

Kneib, J. -P.; Aussel, H.; Taniguchi, Y. +12 more

We report on the stellar content of the COSMOS two degree field, as derived from a rigorous star-galaxy separation approach developed for using stellar sources to define the point-spread function variation map used in a study of weak galaxy lensing. The catalog obtained in one filter from the ACS (Advanced Camera for Surveys on the Hubble Space Te…

2007 The Astrophysical Journal Supplement Series
eHST 26
Solitary Electromagnetic Pulses Detected with Super-Alfvénic Flows in Earth's Geomagnetic Tail
DOI: 10.1103/PhysRevLett.98.265001 Bibcode: 2007PhRvL..98z5001P

Dandouras, I.; Lucek, E.; Rème, H. +11 more

Solitary nonlinear (δB/B≫1) electromagnetic pulses have been detected in Earth’s geomagnetic tail accompanying plasmas flowing at super-Alfvénic speeds. The pulses in the current sheet had durations of ∼5s, were left-hand circularly polarized, and had phase speeds of approximately the Alfvén speed in the plasma frame. These pulses were associated …

2007 Physical Review Letters
Cluster 26
Charged particle environment of Titan during the T9 flyby
DOI: 10.1029/2007GL030677 Bibcode: 2007GeoRL..3424S03S

Coates, A. J.; Crary, F.; Sittler, E. C. +6 more

The ion measurements of the Cassini Plasma Spectrometer are presented which were acquired on 26 December 2005, during the T9 flyby at Titan. The plasma flow and magnetic field directions in the distant plasma environment of the moon were distinctly different from the other flybys. The near-Titan environment, dominated by ions of Titan origin, had …

2007 Geophysical Research Letters
Cassini 26