Search Publications

Synthetic Mid-UV Spectroscopic Indices of Stars
DOI: 10.1086/511295 Bibcode: 2007ApJ...657.1046C

Chavez, M.; Buzzoni, A.; Morossi, C. +4 more

Using the UVBLUE library of synthetic stellar spectra we have computed a set of mid-UV line and continuum spectroscopic indices. We explore their behavior in terms of the leading stellar parameters (Teff, logg). The overall result is that synthetic indices follow the general trends depicted by those computed from empirical databases. Se…

2007 The Astrophysical Journal
IUE 24
Detection of Surface Brightness Fluctuations in Elliptical Galaxies Imaged with the Advanced Camera for Surveys: B- and I-Band Measurements
DOI: 10.1086/517984 Bibcode: 2007ApJ...662..940C

Blakeslee, John P.; Cantiello, Michele; Raimondo, Gabriella +2 more

Taking advantage of the exceptional capabilities of the Advanced Camera for Surveys (ACS) on board the Hubble Space Telescope (HST), we derive surface brightness fluctuation (SBF) measurements in the B and I bands from images of six elliptical galaxies with 1500<=cz<=3500. Given the low signal-to-noise ratio (S/N) of the SBF signal in the bl…

2007 The Astrophysical Journal
eHST 24
The acceleration characteristics of solar energetic particles in the 2000 July 14 event
DOI: 10.1051/0004-6361:20065754 Bibcode: 2007A&A...461.1115L

Li, C.; Dai, Y.; Fang, C. +2 more

Aims:In large gradual solar energetic particle (SEP) events, especially the ground-level enhancement (GLE) events, where and how energetic particles are accelerated is still a problem.
Methods: By using imaging data from TRACE, Yohkoh/HXT, SOHO/MDI and SOHO/EIT, along with the data from the GOES, Apatity NM, and SOHO/LASCO CME catalog, the evo…

2007 Astronomy and Astrophysics
SOHO 24
Huygens’ entry and descent through Titan's atmosphere—Methodology and results of the trajectory reconstruction
DOI: 10.1016/j.pss.2007.04.013 Bibcode: 2007P&SS...55.1845K

Lebreton, Jean-Pierre; Pérez-Ayúcar, Miguel; Sollazzo, Claudio +2 more

The European Space Agency's Huygens probe separated from the NASA Cassini spacecraft on 25 December 2004, after having been attached for a 7-year interplanetary journey and three orbits around Saturn. The probe reached the predefined NASA/ESA interface point on 14 January 2005 at 09:05:52.523 (UTC) and performed a successful entry and descent sequ…

2007 Planetary and Space Science
Huygens 24
Magnetic Solitons: Unified Mechanism for Moving Magnetic Features
DOI: 10.1007/s11207-007-0399-z Bibcode: 2007SoPh..246..281R

Ryutova, M.; Hagenaar, H.

In a highly dynamic environment with sources and sinks of energy, flux tubes do not in general obey local conservation laws, nor do the ensembles of flux tubes that exhibit collective phenomena. We use the approach of energetically open dissipative systems to study nonlinear waves in flux tubes and their role in the dynamics of the overlying atmos…

2007 Solar Physics
SOHO 24
Cassini/Cosmic Dust Analyzer in situ dust measurements between Jupiter and Saturn
DOI: 10.1029/2006JA011978 Bibcode: 2007JGRA..112.7105A

Dikarev, V.; Kempf, S.; Srama, R. +5 more

We report an analysis of the Cosmic Dust Analyzer data obtained during the interplanetary cruise of the Cassini spacecraft between Jupiter and Saturn. The data cover the time period between the Jupiter flyby and the Saturn orbit insertion. Seventeen dust particles on bound and unbound (hyperbolic) orbits were also detected, with sizes in the submi…

2007 Journal of Geophysical Research (Space Physics)
Cassini Ulysses 24
Searching High-Redshift Large-Scale Structures: Photometry of Four Fields around Quasar Pairs at z ~ 1
DOI: 10.1086/519992 Bibcode: 2007ApJ...666..747B

Cypriano, E. S.; West, M.; Santos, W. A. +3 more

We have studied the photometric properties of four fields around the high-redshift quasar pairs QP 1310+0007, QP 1355-0032, QP 0110-0219, and QP 0114-3140 at z~1 with the aim of identifying large-scale structures (galaxy clusters or groups) around them. This sample was observed with the Gemini Multi-Object Spectograph (GMOS) at the Gemini North an…

2007 The Astrophysical Journal
eHST 24
New flaring of an ultraluminous X-ray source in NGC1365
DOI: 10.1111/j.1365-2966.2007.12031.x Bibcode: 2007MNRAS.379.1313S

Zezas, A.; La Parola, V.; Baldi, A. +4 more

We have studied a highly variable ultraluminous X-ray source (ULX) in the Fornax galaxy NGC1365, with a series of 12 Chandra and XMM-Newton observations between 2002 and 2006. In 2006 April, the source peaked at a luminosity ~3 × 1040erg s-1 in the 0.3-10 keV band (similar to the maximum luminosity found by ASCA in 1995), and…

2007 Monthly Notices of the Royal Astronomical Society
XMM-Newton 24
Diagnostics of Radio Fine Structures around 3 GHz with Hinode Data in the Impulsive Phase of an X3.4/4B Flare Event on 2006 December 13
DOI: 10.1093/pasj/59.sp3.S815 Bibcode: 2007PASJ...59S.815Y

Chen, Bin; Sakurai, Takashi; Yan, Yihua +1 more

On 2006 December 13 during the solar minimum, the superactive region NOAA 10930 at the S05W33 disk location produced an X3.4/4B flare at 02:40UT. Fine structures were observed in the radio spectra, which included spikes, reverse slope-type III bursts, type-U burst, V-shaped burst, pulsations, zebra patterns, and firstly discovered sub-second spiky…

2007 Publications of the Astronomical Society of Japan
Hinode SOHO 24
Synchrotron Radio Emission from a Fast Halo Coronal Mass Ejection
DOI: 10.1086/519246 Bibcode: 2007ApJ...665..805B

Bastian, T. S.

An interplanetary (IP) type II-like radio burst is analyzed. It occurred on 2003 June 17-18 in association with a fast halo coronal mass ejection (CME), an M6.8 soft-X-ray (SXR) flare, and it produced a solar proton event. Unlike coronal type II bursts and the majority of IP type II radio emissions, the IP type-II-like event associated with the fa…

2007 The Astrophysical Journal
SOHO 24