Spectroscopy of solar system objects (p. 3) |
by Bezard, B |
The emissivity of mars and Callisto in the far infrared (p. 9) |
by Burgdorf, M J |
ISO spectroscopy of titan (p. 13) |
by Coustenis, A |
The ISO spectra of Uranus and Neptune in the 2.5 - 5.0 micron range (p. 19) |
by Encrenaz, Th |
Circumstellar, cometary and interplanetary dust (p. 23) |
by Crovisier, J |
LWS measurements of HD in the giant planets (p. 29) |
by Davis, G R |
ISO observations of bright asteroids with PHT-S (p. 33) |
by Müller, T G |
The life cycle of dust: an ISO view (p. 39) |
by Waters, L B |
Spectroscopic diversity of the UIR bands as revealed by ISO: Towards a molecular carrier identification (p. 49) |
by Joblin, C |
Unidentified infrared emission bands and far-infrared emission in various interstellar medium (p. 55) |
by Onaka, T |
Characterization of the unidentified infrared emission bands in the diffuse interstellar medium (p. 59) |
by Chan, K W |
The CH out-of â plane bending modes of polycyclic aromatic hydrocarbon molecules in an astrophysical context (p. 63) |
by Hony, S |
Gas-phase H2O and CO2 towards massive protostars (p. 67) |
by Boonman, A M |
Ices around massive young stellar objects : the RAFGL 7009S test case(p. 71) |
by Dartois, E |
The interaction of the galactic center arches cluster and the thermal filaments (p. 77) |
by Cotera, A S |
Molecular spectroscopy with ISO (p. 81) |
by Cernicharo, J |
AIBs and carbon chains in PDRs (p. 91) |
by Fosse, D |
ISO detections of C3 and NH in Sgr B2 (p. 99) |
by Goicoechea, J R |
H2 infrared line emission across the bright side of the Ophiuchi main cloud (p. 103) |
by Habart, H |
C2H2 and HCN toward massive YSO's (p. 107) |
by Lahuis, F |
Ionized bubbles in the galactic center (p. 111) |
by Martín-Pintado, J |
Origin of Si II 35 m and C II 158 m emission in the carina nebula (p. 115) |
by Mizutani, M |
ISO spectroscopy of low Mass outflows and YSOs (p. 123) |
by Noriega-Crespo, A |
Non-equilibrium H2 ortho-to-para ratio in two molecular clouds of the galactic center (p. 127) |
by Rodríguez-Fernández, N J |
Large OI/ CO ratios in cold molecular clouds towards W49N (p. 131) |
by Vastel, C |
ISO spectroscopy of compact H II regions in our galaxy (p. 135) |
by Martin-Hernandez, N L |
The far infrared line spectra of low luminosity protostars (p. 141) |
by Ceccarelli, C |
The ISO atlas of near-infrared stellar spectra and the IR spectral classification of late-type stars (p. 147) |
by Vandenbussche, B |
Crystalline silicates: new probes of circumstellar dust conditions? (p. 151) |
by Molster, F |
Warm gas around AGB stars (p. 155) |
by Yamamura, I |
ISO spectroscopy of AGB stars in the LMC (p. 161) |
by Trams, N R |
ISO spectroscopy of luminous blue variables as a probe of post main sequence massive star evolution (p. 165) |
by Morris, P W |
An infrared/millimeter study of the Dumbell nebula (p. 171) |
by Bachiller, R |
The ISO-SWS line spectrum of planetary nebula NGC 7027 (p. 175) |
by Bernard Salas, J |
Atomic fine-structure lines from protoplanetary nebulae (p. 179) |
by Castro-Carrizo, A |
Composition of the silicates around evolved stars and protostars (p. 183) |
by Demyk, K |
ISO SWS spectroscopy of carbon-rich proto-planetary nebulae (p. 191) |
by Hrivnak, B J |
Water vapour in cool dwarf stars (p. 195) |
by Jones, H |
On the mineralogy of oxygen-rich AGB variables (p. 203) |
by Kerschbaum, F |
Infrared Teff calibration of late-O and early-B stars with ISO-SWS (p. 207) |
by De Koter, A |
Infrared 2.4 - 4.1 micron spectra of OB-type stars (p. 211) |
by Lenorzer, A |
ISO LWS-SWS observation of IRAS 19120+1103 (p. 215) |
by Leto, G |
ISO-SWS observations on proto-planetary system candidates (p. 219) |
by Palacios, J |
The C-C-C- bending modes of PAHs: A new emission plateau from 15 to 20 (p. 223) |
by Van Kerckhoven, C |
Spectral variations in R CrB stars (p. 227) |
by Walker, H J |
Galaxies: The short wavelength view (p. 233) |
by Lutz, D |
PHT-S spectroscopy of Seyfert galaxies (p. 245) |
by Schulz, B |
C II 158 $\mu$m observations of a sample of late-type galaxies from the Virgo cluster (p. 257) |
by Leech, K J |
ISO spectroscopy of seyfert galaxies: fine structure line diagnostics in seven galaxies (p. 261) |
by Spignolo, L |
Update on ISO instruments calibration and data analysis techniques (p. 267) |
by García-Lario, P |
NGC 7027: A comparison of ISOCAM CVF and ground-based mid-infrared CVF images (p. 273) |
by Ali, B |
Improving the SWS spectrum of titan - correcting for the reset pulse aftermath (p. 275) |
by Kester, D |
A simple approach to LWS memory effects description (p. 279) |
by Pezzuto, S |
Recovery of non-prime Fabry-Perot data in the LWS (p. 283) |
by Polehampton, E T |
A new generation of dynamical models for long-period variables: a new era for the interpretation of ISO-SWS data of cool giants (p. 295) |
by Aringer, B |
A new generation of model atmospheres for AGB stars inspired by ISO (p. 299) |
by Höfner, S |
Radiative transfer: progress and problems (p. 303) |
by Ossenkopf, V |
Modeling line emission in PDRs (p. 309) |
by Le Bourlot, J |
Probing the outer atmosphere of carbon stars - C2H2, HCN and C3 features in the SWS range (p. 315) |
by Loidl, R |
Shapes of dust features in carbon-rich sources (p. 323) |
by Volk, K |
Infrared spectroscopy of cosmic grains - contributions from laboratory astrophysics (p. 329) |
by Henning, T |
High-temperature crystallization of silicate dust (p. 335) |
by Brucato, J R |
16-80 spectra of crystalline silicates at 4 K, 80 K and 295 K (p. 339) |
by Bowey, J E |
Causes of artifacts in the infrared spectra of powders (p. 343) |
by Hofmeister, A M |
Amorphous to crystalline transition of magnesium silicate and silica nanoparticles (p. 347) |
by Fabian, D |
Sciences opportunities with SIRTF (p. 353) |
by Gehrz, R D |
Astro-F: infrared imaging surveyor (IRIS) mission (p. 361) |
by Onaka, T |
Future IR/submm space missions (p. 365) |
by De Graauw, T |
Conference summary (p. 373) |
by Cernicharo, J |