Search Publications

Quasi-perpendicular Shock Structure and Processes
DOI: 10.1007/s11214-005-3827-0 Bibcode: 2005SSRv..118..161B

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

2005 Space Science Reviews
Cluster 150
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
The Ice Survey Opportunity of ISO
DOI: 10.1007/s11214-005-8059-9 Bibcode: 2005SSRv..119..293D

Dartois, Emmanuel

The instruments on board the Infrared Space Observatory have for the first time allowed a complete low (PHOT, CVF) to medium resolution (SWS) spectroscopic harvest, from 2.5 to 45 µm, of interstellar dust. Amongst the detected solids present in starless molecular clouds surrounding recently born stellar and still embedded objects or products…

2005 Space Science Reviews
ISO 104
The Magnetosheath
DOI: 10.1007/s11214-005-3825-2 Bibcode: 2005SSRv..118...95L

Sahraoui, F.; Lucek, E. A.; Walker, S. N. +5 more

2005 Space Science Reviews
Cluster 96
Crystalline Silicates
DOI: 10.1007/s11214-005-8066-x Bibcode: 2005SSRv..119....3M

Kemper, Ciska; Molster, Frank

One of the big surprises of the Infrared Space Observatory (ISO) has been discovery of crystalline silicates outside our own Solar system. It was generally assumed before that all cosmic silicates in space were of amorphous structure. Thanks to ISO we know now that crystalline silicates are ubiquitous in the Galaxy (except for the diffuse ISM) and…

2005 Space Science Reviews
ISO 94
Magnetopause and Boundary Layer
DOI: 10.1007/s11214-005-3834-1 Bibcode: 2005SSRv..118..231D

Lundin, R.; Vaivads, A.; Owen, C. J. +6 more

2005 Space Science Reviews
Cluster 56
Molecular Hydrogen
DOI: 10.1007/s11214-005-8062-1 Bibcode: 2005SSRv..119...71H

Maiolino, Roberto; Habart, Emilie; Walmsley, Malcolm +5 more

Observations of H2 line emission in galactic and extragalactic environments obtained with the Infrared Space Observatory (ISO) are reviewed. The diagnostic capability of H2 observations is illustrated. We discuss what one has learned about such diverse astrophysical sources as photon-dominated regions, shocks, young stellar o…

2005 Space Science Reviews
ISO 50
Deep Impact: Working Properties for the Target Nucleus Comet 9P/Tempel 1
DOI: 10.1007/s11214-005-3389-1 Bibcode: 2005SSRv..117..137B

Fernández, Yanga R.; A'Hearn, Michael F.; Pittichová, Jana +13 more

In 1998, Comet 9P/Tempel 1 was chosen as the target of the Deep Impact mission (A’Hearn, M. F., Belton, M. J. S., and Delamere, A., Space Sci. Rev., 2005) even though very little was known about its physical properties. Efforts were immediately begun to improve this situation by the Deep Impact Science Team leading to the founding of a worldwide o…

2005 Space Science Reviews
eHST 49
Obscured Activity: AGN, Quasars, Starbursts and ULIGs Observed by the Infrared Space Observatory
DOI: 10.1007/s11214-005-8072-z Bibcode: 2005SSRv..119..355V

Haas, Martin; Klaas, Ulrich; Lutz, Dieter +2 more

Some of the most ‘active’ galaxies in the Universe are obscured by large quantities of dust and emit a substantial fraction of their bolometric luminosity in the infrared. Observations of these infrared luminous galaxies with the Infrared Space Observatory (ISO) have provided a relatively unabsorbed view to the sources fuelling this active emissio…

2005 Space Science Reviews
ISO 49
Water in Space: The Water World of ISO
DOI: 10.1007/s11214-005-8058-x Bibcode: 2005SSRv..119...29C

Cernicharo, José; Crovisier, Jacques

In this review we present the main results obtained by the ISO satellite on the abundance and spatial distribution of water vapor in the direction of molecular clouds, evolved stars, galaxies, and in the bodies of our Solar System. We also discuss the modeling of H2O and the difficulties found in the interpretation of the data, the need…

2005 Space Science Reviews
ISO 48