Search Publications

Astrophysical parameters of Galactic open clusters
DOI: 10.1051/0004-6361:20042523 Bibcode: 2005A&A...438.1163K

Scholz, R. -D.; Piskunov, A. E.; Kharchenko, N. V. +2 more

We present a catalogue of astrophysical data for 520 Galactic open clusters. These are the clusters for which at least three most probable members (18 on average) could be identified in the ASCC-2.5, a catalogue of stars based on the Tycho-2 observations from the Hipparcos mission. We applied homogeneous methods and algorithms to determine angular…

2005 Astronomy and Astrophysics
Hipparcos 604
In situ measurements of the physical characteristics of Titan's environment
DOI: 10.1038/nature04314 Bibcode: 2005Natur.438..785F

Neubauer, F. M.; Rodrigo, R.; Barucci, M. A. +40 more

On the basis of previous ground-based and fly-by information, we knew that Titan's atmosphere was mainly nitrogen, with some methane, but its temperature and pressure profiles were poorly constrained because of uncertainties in the detailed composition. The extent of atmospheric electricity (`lightning') was also hitherto unknown. Here we report t…

2005 Nature
Huygens 542
Wave acceleration of electrons in the Van Allen radiation belts
DOI: 10.1038/nature03939 Bibcode: 2005Natur.437..227H

Meredith, Nigel P.; Horne, Richard B.; Glauert, Sarah A. +11 more

The Van Allen radiation belts are two regions encircling the Earth in which energetic charged particles are trapped inside the Earth's magnetic field. Their properties vary according to solar activity and they represent a hazard to satellites and humans in space. An important challenge has been to explain how the charged particles within these bel…

2005 Nature
Cluster 493
Spitzer View on the Evolution of Star-forming Galaxies from z = 0 to z ~ 3
DOI: 10.1086/431894 Bibcode: 2005ApJ...630...82P

Papovich, Casey; Pérez-González, Pablo G.; Rieke, George H. +11 more

We use a 24 µm-selected sample containing more than 8000 sources to study the evolution of star-forming galaxies in the redshift range from z=0 to z~3. We obtain photometric redshifts for most of the sources in our survey using a method based on empirically built templates spanning from ultraviolet to mid-infrared wavelengths. The accuracy o…

2005 The Astrophysical Journal
eHST 485
The Effective Temperature Scale of FGK Stars. II. Teff:Color:[Fe/H] Calibrations
DOI: 10.1086/430102 Bibcode: 2005ApJ...626..465R

Meléndez, Jorge; Ramírez, Iván

We present up-to-date metallicity-dependent temperature versus color calibrations for main-sequence and giant stars based on temperatures derived with the infrared flux method (IRFM). Seventeen colors in the photometric systems UBV, uvby, Vilnius, Geneva, RI(Cousins), DDO, Hipparcos-Tycho, and Two Micron All Sky Survey (2MASS) have been calibrated…

2005 The Astrophysical Journal
Hipparcos 485
Optimization of Starburst99 for Intermediate-Age and Old Stellar Populations
DOI: 10.1086/427866 Bibcode: 2005ApJ...621..695V

Leitherer, Claus; Vázquez, Gerardo A.

We have incorporated the latest release of the Padova models into the evolutionary synthesis code Starburst99. The Padova tracks were extended to include the full asymptotic giant branch (AGB) evolution until the final thermal pulse over the mass range 0.9-5 Msolar. With this addition, Starburst99 accounts for all stellar phases that co…

2005 The Astrophysical Journal
eHST 478
The afterglow of GRB 050709 and the nature of the short-hard γ-ray bursts
DOI: 10.1038/nature04189 Bibcode: 2005Natur.437..845F

Cenko, S. B.; Peterson, B. A.; Price, P. A. +33 more

The final chapter in the long-standing mystery of the γ-ray bursts (GRBs) centres on the origin of the short-hard class of bursts, which are suspected on theoretical grounds to result from the coalescence of neutron-star or black-hole binary systems. Numerous searches for the afterglows of short-hard bursts have been made, galvanized by the revolu…

2005 Nature
eHST 478
Measurement of the Electric Fluctuation Spectrum of Magnetohydrodynamic Turbulence
DOI: 10.1103/PhysRevLett.94.215002 Bibcode: 2005PhRvL..94u5002B

Bale, S. D.; Horbury, T. S.; Reme, H. +2 more

Magnetohydrodynamic (MHD) turbulence in the solar wind is observed to show the spectral behavior of classical Kolmogorov fluid turbulence over an inertial subrange and departures from this at short wavelengths, where energy should be dissipated. Here we present the first measurements of the electric field fluctuation spectrum over the inertial and…

2005 Physical Review Letters
Cluster 476
The Solar Wind as a Turbulence Laboratory
DOI: 10.12942/lrsp-2005-4 Bibcode: 2005LRSP....2....4B

Bruno, Roberto; Carbone, Vincenzo

In this review we will focus on a topic of fundamental importance for both plasma physics and astrophysics, namely the occurrence of large-amplitude low-frequency fluctuations of the fields that describe the plasma state. This subject will be treated within the context of the expanding solar wind and the most meaningful advances in this research f…

2005 Living Reviews in Solar Physics
Ulysses 476
Toward an Understanding of the Rapid Decline of the Cosmic Star Formation Rate
DOI: 10.1086/429552 Bibcode: 2005ApJ...625...23B

Papovich, Casey; Pérez-González, Pablo G.; Bell, Eric F. +11 more

We present a first analysis of deep 24 µm observations with the Spitzer Space Telescope of a sample of nearly 1500 galaxies in a thin redshift slice, 0.65<=z<0.75. We combine the infrared data with redshifts, rest-frame luminosities, and colors from COMBO-17 and with morphologies from Hubble Space Telescope images collected by the Gala…

2005 The Astrophysical Journal
eHST 471