Search Publications

Direction of the interstellar H atom inflow in the heliosphere: Role of the interstellar magnetic field
DOI: 10.1051/0004-6361:200500132 Bibcode: 2005A&A...437L..35I

Izmodenov, V.; Alexashov, D.; Myasnikov, A.

Recently Lallement et al. (2005, Science, 307, 1447) reported that the direction of the flow of interstellar neutral hydrogen in the heliosphere is deflected by ~4° from the direction of the pristine local interstellar gas flow. The most probable physical phenomenon responsible for such a deviation is the interstellar magnetic field inclined to th…

2005 Astronomy and Astrophysics
SOHO 146
Visibility of coronal mass ejections as a function of flare location and intensity
DOI: 10.1029/2005JA011151 Bibcode: 2005JGRA..11012S05Y

Howard, R. A.; Gopalswamy, N.; Michalek, G. +2 more

We report the visibility (detection efficiency) of coronal mass ejections (CMEs) of the Large Angle Spectrometric Coronagraph (LASCO) on board the Solar and Heliospheric Observatory (SOHO). We collected 1301 X-ray flare events (above C3 level) detected by the GOES satellite and examined their CME associations using data from LASCO coronagraphs. Th…

2005 Journal of Geophysical Research (Space Physics)
SOHO 145
Compositional maps of Saturn's moon Phoebe from imaging spectroscopy
DOI: 10.1038/nature03558 Bibcode: 2005Natur.435...66C

Sotin, C.; Baines, K. H.; Nicholson, P. D. +23 more

The origin of Phoebe, which is the outermost large satellite of Saturn, is of particular interest because its inclined, retrograde orbit suggests that it was gravitationally captured by Saturn, having accreted outside the region of the solar nebula in which Saturn formed. By contrast, Saturn's regular satellites (with prograde, low-inclination, ci…

2005 Nature
Cassini 145
The Evolution and Structure of Early-Type Field Galaxies: A Combined Statistical Analysis of Gravitational Lenses
DOI: 10.1086/427908 Bibcode: 2005ApJ...623..666R

Kochanek, C. S.; Rusin, D.

We introduce a framework for simultaneously investigating the structure and luminosity evolution of early-type gravitational lens galaxies. The method is based on the fundamental plane, which we interpret using the aperture mass-radius relations derived from lensed image geometries. We apply this method to our previous sample of 22 lens galaxies w…

2005 The Astrophysical Journal
eHST 144
Abundance trends in kinematical groups of the Milky Way's disk
DOI: 10.1051/0004-6361:20042390 Bibcode: 2005A&A...438..139S

Soubiran, C.; Girard, P.

We have compiled a large catalogue of metallicities and abundance ratios from the literature in order to investigate abundance trends of several alpha and iron peak elements in the thin disk and the thick disk of the Galaxy. The catalogue includes 743 stars with abundances of Fe, O, Mg, Ca, Ti, Si, Na, Ni and Al in the metallicity range -1.30 <…

2005 Astronomy and Astrophysics
Hipparcos 143
Mapping the Kinematics of the Narrow-Line Region in the Seyfert Galaxy NGC 4151
DOI: 10.1086/432255 Bibcode: 2005AJ....130..945D

Gull, T. R.; Kraemer, S. B.; Crenshaw, D. M. +6 more

Using the Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph (STIS), observations of the [O III] emission from the narrow-line region (NLR) of NGC 4151 were obtained and radial velocities determined. Five orbits of HST time were used to obtain spectra at five parallel slit configurations at a position angle of 58°, with spatial reso…

2005 The Astronomical Journal
eHST 143
Discovery of 10 µm silicate emission in quasars. Evidence of the AGN unification scheme
DOI: 10.1051/0004-6361:200500109 Bibcode: 2005A&A...436L...5S

Siebenmorgen, R.; Schulz, B.; Haas, M. +1 more

According to the unified scheme, AGN are surrounded by a dust-torus, and the observed diversity of AGN properties results from the different orientations relative to our line of sight. The strong resonance of silicate dust at 10 µm is therefore, as expected, seen in absorption towards many type-2 AGN. In type-1 AGN, it should be seen in emis…

2005 Astronomy and Astrophysics
ISO 143
Spitzer imaging of i'-drop galaxies: old stars at z~ 6
DOI: 10.1111/j.1365-2966.2005.09434.x Bibcode: 2005MNRAS.364..443E

Bunker, Andrew J.; Ellis, Richard S.; Stanway, Elizabeth R. +3 more

We present new evidence for mature stellar populations with ages >100Myr in massive galaxies (Mstellar > 1010Msolar) seen at a time when the Universe was less than 1Gyr old. We analyse the prominent detections of two z~ 6 star-forming galaxies (SBM03#1 and #3) made at wavelengths corresponding to the rest-fra…

2005 Monthly Notices of the Royal Astronomical Society
eHST 142
Evidence from the Mars Express High Resolution Stereo Camera for a frozen sea close to Mars' equator
DOI: 10.1038/nature03379 Bibcode: 2005Natur.434..352M

HRSC Co-Investigator Team; Head, James W.; van Gasselt, Stephan +10 more

It is thought that the Cerberus Fossae fissures on Mars were the source of both lava and water floods two to ten million years ago. Evidence for the resulting lava plains has been identified in eastern Elysium, but seas and lakes from these fissures and previous water flooding events were presumed to have evaporated and sublimed away. Here we pres…

2005 Nature
MEx 142
Can the Steep Mass Profile of A1689 Be Explained by a Triaxial Dark Halo?
DOI: 10.1086/452629 Bibcode: 2005ApJ...632..841O

Broadhurst, Tom; Oguri, Masamune; Umetsu, Keiichi +1 more

The steep mass profile of A1689 derived from recent detailed lensing observations is not readily reconciled with the low-concentration halos predicted by the standard cold dark matter (CDM) model. However, halo triaxiality may act to bias the profile constraints derived assuming a spherically symmetric mass distribution, since lensing relates only…

2005 The Astrophysical Journal
eHST 141