Search Publications

Ultraviolet images of galaxies from the Optical Monitor on XMM-Newton
DOI: 10.1016/j.asr.2003.02.079 Bibcode: 2004AdSpR..34.2540B

Kaastra, J. S.; Branduardi-Raymont, G.; Kahn, S. M. +3 more

A large number of galaxies, both normal and active, have been observed in ultraviolet light by the Optical Monitor on XMM-Newton. These are some of the deepest wide-field ultraviolet images of these galaxies yet obtained, and in many cases the first collected in this waveband. We present images of five active galaxies, and discuss the potential us…

2004 Advances in Space Research
XMM-Newton 0
Environmental predictions for the Beagle 2 lander, based on GCM climate simulations
DOI: 10.1016/j.pss.2003.12.001 Bibcode: 2004P&SS...52..259B

Newman, C. E.; Lewis, S. R.; Read, P. L. +1 more

The Mars climate database (MCD) is a database of statistics based on output from physically consistent numerical model simulations which describe the climate and surface environment of Mars. It is used here to predict the meteorological environment of the Beagle 2 lander site. The database was constructed directly on the basis of output from multi…

2004 Planetary and Space Science
MEx 0
Infrared Space Observatory Observations of the 53W002 Group at 6.7 Microns: In Search of the Oldest Stellar Populations at z = 2.4
DOI: 10.1086/423432 Bibcode: 2004PASP..116..712K

Keel, William C.; Windhorst, Rogier A.; Eales, Stephen A. +5 more

We present a deep Infrared Space Observatory (ISO) observation at 6.7 µm of the 53W002 group of galaxies and active galactic nuclei (AGNs) at z=2.4. This approximately samples the emitted K band. Faint, blue star-forming objects are not detected, as expected from their very blue color across the emitted optical and UV spectrum. However, 53W0…

2004 Publications of the Astronomical Society of the Pacific
ISO eHST 0
Abundancias químicas y estado de evolución de estrellas tipo B y A
Bibcode: 2004BAAA...47..102P

Adelman, S. J.; Pintado, O.; Pedrosa, S.

Three stars of B (Alpha Tel and HR1781) and A (Tau7 Eri) type have been studied in order to determine their evolutionary state and the presence of chemical peculiarities. For this study we used spectra with high signal-to-noise ratios, obtained with the EBASIM spectrograph at CASLEO. The efective temperature, surface gravity, rotational velocity a…

2004 Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
Hipparcos 0
XMM-Newton Observations of the Poor Cluster MKW 4
Bibcode: 2004cgpc.sympE..40O

O'Sullivan, E.

We present a 15 ksec observation of the poor cluster MKW 4. While the cluster itself appears to be relaxed with little X-ray substructure, it is dominated by NGC 4073, a cD galaxy with a kinematically distinct core. We investigate the structure and properties of the cluster halo with particular reference to the temperature and abundance distributi…

2004 Clusters of Galaxies: Probes of Cosmological Structure and Galaxy Evolution
XMM-Newton 0
Small Main-belt Asteroid Spectroscopic Survey, Phase II
Bibcode: 2004PDSS....1.....B

Binzel, R. P.; Bus, S.

This data set contains visible-wavelength (0.435-0.925 micron) spectra for 1341 main-belt asteroids observed during the second phase of the Small Main-belt Asteroid Spectroscopic Survey (SMASSII) between August 1993 and March 1999. The purpose of the SMASSII survey was to provide a new basis for studying the compositional diversity and structure o…

2004 NASA Planetary Data System
Hipparcos 0
Interplanetary Disturbances
DOI: 10.1007/978-3-540-31534-6_4 Bibcode: 2004LNP...656...71W

Wimmer-Schweingruber, Robert F.

The Sun emits the variable solar wind which interacts with the very local interstellar medium to form the heliosphere. Hence variations in solar activity strongly influence interplanetary space, from the Suns surface out to the edge of the heliosphere. Superimposed on the solar wind are mass ejections from the Sun and/or its corona which disturb t…

2004 Lecture Notes in Physics, Berlin Springer Verlag
Ulysses 0
Mid-Infrared properties of Early-type galaxies
DOI: 10.1023/B:ASTR.0000014972.15891.9b Bibcode: 2004Ap&SS.289..415X

Madden, S. C.; Vigroux, L.; Xilouris, E. M.

We have conducted a survey of early-type galaxies using the ISOCAMinstrument on board the Infrared Space Observatory (ISO)in order to probe their dustcontent. We present Mid-Infrared photometric properties for a sampleof 20 galaxies observed at 4.5, 7 and 15 µ$m. Using diagnosticcolor-color diagrams, we can delineate the different Mid-Infrar…

2004 Astrophysics and Space Science
ISO 0
Multiple Flux Rope Events at the High-Latitude Magnetopause: Cluster/Rapid Observation on January 26, 2001
Bibcode: 2004ChJG...47.2634H

Reme, H.; Cao, Jin-Bin; Daly, P. +15 more

From 11:10 to 11:40UT on January 26, 2001 the four Cluster II spacecraft were located in the duskside high latitude regions of the magnetosheath and magnetosheath boundary layer (MSBL). During this time Interval the interplanetary magnetic field (IMF) had a negative Bz component. A detailed study on the multiple flux ropes (MFRs) observed in this …

2004 Chinese Journal of Geophysics
Cluster 0
La Cometa 67P Churyumov-Gerasimenko el il contributo degli astrofili italiani alla missione ROSETTA
Bibcode: 2004AsUAI...4...54M

Milani, Giannantonio

Comet 67P Churyumov-Gerasimenko, the new target of the ROSETTA spacecraft, was oberved during the 2002/2003 apparition, displacing an unusual tail. The tail was compatible with a neck-line structure and this implies a high nuclear activity far before perihelion. Images and data from the current and previous apparitions show that the comet reaches …

2004 Astronomia. La rivista dell' Unione Astrofili Italiani
Rosetta 0