Search Publications

Cosmic Evolution of Stellar Disk Truncations: From z ~ 1 to the Local Universe
DOI: 10.1086/590142 Bibcode: 2008ApJ...684.1026A

Beckman, J. E.; Trujillo, I.; Azzollini, R.

We have conducted the largest systematic search so far for stellar disk truncations in disklike galaxies at intermediate redshift (z < 1.1), using the Great Observatories Origins Deep Survey-South (GOODS-S) data from the Hubble Space Telescope ACS. Focusing on type II galaxies (i.e., downbending profiles), we explore whether the position of the…

2008 The Astrophysical Journal
eHST 52
A Spectroscopic Orbit for Regulus
DOI: 10.1086/591148 Bibcode: 2008ApJ...682L.117G

Rivinius, Th.; Štefl, S.; Baade, D. +8 more

We present a radial velocity study of the rapidly rotating B star Regulus that indicates the star is a single-lined spectroscopic binary. The orbital period (40.11 days) and probable semimajor axis (0.35 AU) are large enough that the system is not interacting at present. However, the mass function suggests that the secondary has a low mass (M

2008 The Astrophysical Journal
IUE 52
Cassini UVIS observations of the Io plasma torus. IV. Modeling temporal and azimuthal variability
DOI: 10.1016/j.icarus.2007.09.019 Bibcode: 2008Icar..194..153S

Delamere, P. A.; Bagenal, F.; Steffl, A. J.

In this fourth paper in a series, we present a model of the remarkable temporal and azimuthal variability of the Io plasma torus observed during the Cassini encounter with Jupiter. Over a period of three months, the Cassini Ultraviolet Imaging Spectrograph (UVIS) observed a dramatic variation in the average torus composition. Superimposed on this …

2008 Icarus
Cassini 52
Stratigraphy and structure of interior layered deposits in west Candor Chasma, Mars, from High Resolution Stereo Camera (HRSC) stereo imagery and derived elevations
DOI: 10.1029/2007JE003053 Bibcode: 2008JGRE..11310008F

Scholten, F.; Neukum, G.; Hauber, E. +5 more

Interior layered deposits (ILDs) within western Candor Chasma were studied by mapping lithologies, measuring layer attitudes and comparing the stratigraphy of two adjacent mounds. Layering tends to dip in the same direction as the local topographic slope, although at different angles. Regionally consistent attitudes do exist, suggesting postdeposi…

2008 Journal of Geophysical Research (Planets)
MEx 52
AKARI Near-Infrared Spectroscopy: Detection of H2O and CO2 Ices toward Young Stellar Objects in the Large Magellanic Cloud
DOI: 10.1086/592948 Bibcode: 2008ApJ...686L..99S

Onaka, Takashi; Ita, Yoshifusa; Sakon, Itsuki +4 more

We present the first results of AKARI Infrared Camera near-infrared spectroscopic survey of the Large Magellanic Cloud (LMC). We detected absorption features of the H2O ice 3.05 µm and the CO2 ice 4.27 µm stretching mode toward seven massive young stellar objects (YSOs). These samples are for the first time spectr…

2008 The Astrophysical Journal
AKARI 52
Spitzer Observations of Star Formation in the Extreme Outer Disk of M83 (NGC5236)
DOI: 10.1088/0004-6256/136/1/479 Bibcode: 2008AJ....136..479D

Meurer, Gerhardt R.; Calzetti, Daniela; Walter, Fabian +4 more

Spitzer Infrared Array Camera (IRAC) observations of two fields in the extended UV disk (XUV-disk) of M83 have been recently obtained, ~3 R HII away from the center of the galaxy (R HII = 6.6 kpc). Galaxy Evolution Explorer (GALEX) UV images have shown the two fields to host in situ recent star formation. The IRAC images are …

2008 The Astronomical Journal
eHST 52
Influence of Low-Degree High-Order p-Mode Splittings on the Solar Rotation Profile
DOI: 10.1007/s11207-008-9144-5 Bibcode: 2008SoPh..251..119G

Eff-Darwich, A.; Korzennik, S. G.; Jiménez-Reyes, S. J. +3 more

The solar rotation profile is well constrained down to about 0.25R thanks to the study of acoustic modes. Since the radius of the inner turning point of a resonant acoustic mode is inversely proportional to the ratio of its frequency to its degree, only the low-degree p modes reach the core. The higher the order of these modes, the dee…

2008 Solar Physics
SOHO 51
Field Line Shrinkage in Flares Observed by the X-Ray Telescope on Hinode
DOI: 10.1086/526336 Bibcode: 2008ApJ...675..868R

Reeves, Katharine K.; Forbes, Terry G.; Seaton, Daniel B.

The X-Ray Telescope on Hinode has observed individual loops of plasma moving downward in a manner that is consistent with field line shrinkage in the aftermath of reconnection at higher altitudes. An on-disk B3.8 flare observed on 2007 May 2 has loops that clearly change in shape from cusp-shaped to more rounded. In addition, bright loops are obse…

2008 The Astrophysical Journal
Hinode 51
Furthering our understanding of electrostatic solitary waves through Cluster multispacecraft observations and theory
DOI: 10.1016/j.asr.2007.05.064 Bibcode: 2008AdSpR..41.1666P

Gurnett, D. A.; Lakhina, G. S.; Tsurutani, B. T. +9 more

Nonlinear isolated electrostatic solitary waves (ESWs) are observed routinely at many of Earth’s major boundaries by the Wideband Data (WBD) plasma wave receivers that are mounted on the four Cluster satellites. The current study discusses two aspects of ESWs: their characteristics in the magnetosheath, and their propagation in the magnetosheath a…

2008 Advances in Space Research
Cluster 51
Chandra Observations of the Pulsar B1929+10 and Its Environment
DOI: 10.1086/590949 Bibcode: 2008ApJ...685.1129M

Garmire, G. P.; Pavlov, G. G.; Misanovic, Z.

We report on two Chandra observations of the 3 Myr old pulsar B1929+10, which reveal a faint compact (~9'' × 5'') nebula elongated in the direction perpendicular to the pulsar's proper motion, two patchy wings, and a possible short (~3'') jet emerging from the pulsar. In addition, we detect a tail extending up to a…

2008 The Astrophysical Journal
XMM-Newton 51