Search Publications

What Is the Neon Abundance of the Sun?
DOI: 10.1086/431926 Bibcode: 2005ApJ...631.1281B

Basu, Sarbani; Bahcall, John N.; Serenelli, Aldo M.

We have evolved a series of 13 complete solar models that utilize different assumed heavy-element compositions. Models that are based upon the heavy-element abundances recently determined by Asplund and coworkers are inconsistent with helioseismological measurements. However, models in which the neon abundance is increased by 0.4-0.5 dex to logN(N…

2005 The Astrophysical Journal
SOHO 125
Quasi-parallel Shock Structure and Processes
DOI: 10.1007/s11214-005-3832-3 Bibcode: 2005SSRv..118..205B

Balogh, A.; Thomsen, M. F.; Lembège, B. +11 more

2005 Space Science Reviews
Cluster 122
Observational Evidence of the Kink Instability in Solar Filament Eruptions and Sigmoids
DOI: 10.1086/429379 Bibcode: 2005ApJ...622L..69R

Rust, D. M.; LaBonte, B. J.

Two lines of observational evidence are used to infer that the MHD helical kink instability is associated with solar eruptions. The senses of twist and writhe are determined in images of seven erupting filaments obtained at 10830, 1600, 195, and 171 Å. In every case the sense of twist is the same as the sense of writhe, as required for a kink. Fro…

2005 The Astrophysical Journal
SOHO 122
Probing the Environment in Gamma-Ray Bursts: The Case of an X-Ray Precursor, Afterglow Late Onset, and Wind Versus Constant Density Profile in GRB 011121 and GRB 011211
DOI: 10.1086/428377 Bibcode: 2005ApJ...623..314P

Piro, L.; Frontera, F.; Costa, E. +9 more

In this paper we present BeppoSAX and XMM-Newton observations of two long gamma-ray bursts (GRBs), the X-ray-rich event of 2001 December 11 (GRB 011211) and the hard and very bright event of 2001 November 21 (GRB 011121). In both events we find evidence of a late X-ray burst taking place several minutes after the prompt emission. In the November b…

2005 The Astrophysical Journal
XMM-Newton 121
Gamma-ray continuum emission from the inner Galactic region as observed with INTEGRAL/SPI
DOI: 10.1051/0004-6361:20053798 Bibcode: 2005A&A...444..495S

Strong, A. W.; Bouchet, L.; Terrier, R. +5 more

The diffuse continuum emission from the Galactic plane in the energy range 18-1000 keV has been studied using 16 Ms of data from the SPI instrument on INTEGRAL. With such an exposure we can exploit the imaging properties of SPI to achieve a good separation of point sources from the various diffuse components. Using a candidate-source catalogue der…

2005 Astronomy and Astrophysics
INTEGRAL 121
Flow discharge and sediment transport models for estimating a minimum timescale of hydrological activity and channel and delta formation on Mars
DOI: 10.1029/2005JE002521 Bibcode: 2005JGRE..11012003K

Kleinhans, M. G.

This paper summarizes state-of-the-art models for water flow and sediment transport and suggests implications for the sediment grain size distribution, transport process, and delta formation. The flow velocity in Martian outflow channels is commonly calculated from the Manning equation, which is dimensionally incorrect and masks the large uncertai…

2005 Journal of Geophysical Research (Planets)
MEx 121
The Evolution of Early-Type Red Galaxies with the GEMS Survey: Luminosity-Size and Stellar Mass-Size Relations Since z=1
DOI: 10.1086/432786 Bibcode: 2005ApJ...632..191M

Bell, Eric F.; Somerville, Rachel S.; Wisotzki, Lutz +14 more

We combine imaging from the Hubble Space Telescope Advanced Camera for Surveys, as part of the GEMS (Galaxy Evolution from Morphologies and SEDs) survey, with redshifts and rest-frame quantities from COMBO-17 to study the evolution of morphologically early-type galaxies with red colors since z=1. From 0.5d×0.5d imaging, we draw a large sample of 7…

2005 The Astrophysical Journal
eHST 120
Hubble Space Telescope Advanced Camera for Surveys Coronagraphic Imaging of the AU Microscopii Debris Disk
DOI: 10.1086/426755 Bibcode: 2005AJ....129.1008K

Ford, H. C.; Demarco, R.; Infante, L. +38 more

We present Hubble Space Telescope Advanced Camera for Surveys multicolor coronagraphic images of the recently discovered edge-on debris disk around the nearby (~10 pc) M dwarf AU Microscopii. The disk is seen between r=0.75" and 15" (7.5-150 AU) from the star. It has a thin midplane with a projected FWHM thickness of 2.5-3.5 AU within r<50 AU o…

2005 The Astronomical Journal
eHST 119
Evolution and rotation of large-scale photospheric magnetic fields of the Sun during cycles 21-23. Periodicities, north-south asymmetries and r-mode signatures
DOI: 10.1051/0004-6361:20042091 Bibcode: 2005A&A...438.1067K

Stenflo, J. O.; Berdyugina, S. V.; Knaack, R.

We present the results of an extensive time series analysis of longitudinally-averaged synoptic maps, recorded at the National Solar Observatory (NSO/Kitt Peak) from 1975 to 2003, and provide evidence for a multitude of quasi-periodic oscillations in the photospheric magnetic field of the Sun. In the low frequency range, we have located the source…

2005 Astronomy and Astrophysics
SOHO 119
A study of the Type II-P supernova 2003gd in M74
DOI: 10.1111/j.1365-2966.2005.08928.x Bibcode: 2005MNRAS.359..906H

Smartt, S. J.; Peletier, R. F.; Kotak, R. +18 more

We present photometric and spectroscopic data of the Type II-P supernova (SN II-P) 2003gd, which was discovered in M74 close to the end of its plateau phase. SN 2003gd is the first Type II supernova (SN) to have a directly confirmed red supergiant (RSG) progenitor. We compare SN 2003gd to SN 1999em, a similar SN II-P, and estimate an explosion dat…

2005 Monthly Notices of the Royal Astronomical Society
eHST 119