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1.

図書

図書
editors, W. Kinsner, A, Sebak, and K. Ferens
出版情報: Piscataway, N.J. : Institute of Electrical and Electronics Engineers, c2002  3 v. (S.46, 1657 p.) ; 28 cm
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2.

図書

図書
issued by International Institute of Refrigeration ; [editor, Kostadin Fikiin] = edité par Institut International du Froid
出版情報: Paris : Institut International du Froid, c2000  701 p. ; 24 cm
シリーズ名: Science et technique du froid = Refrigeration science and technology ; 1998-6
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3.

図書

図書
editors
出版情報: Montreal, Québec : Canadian Society for Civil Engineering, [2001]  1 v. (various paging) ; 22 cm
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4.

図書

図書
International Institute of Refrigeration
出版情報: Paris : Institut International du Froid, c2001  23 p. ; 30 cm
シリーズ名: Tables and diagrams for the refrigeration industry = Tables et diagrammes pour l'industrie du froid
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5.

図書

図書
International Institute of Refrigeration
出版情報: Paris : Institut International du Froid, c2001  23 p. ; 30 cm
シリーズ名: Tables and diagrams for the refrigeration industry = Tables et diagrammes pour l'industrie du froid
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6.

図書

図書
International Institute of Refrigeration
出版情報: Paris : Institut International du Froid, c2001  21 p. ; 30 cm
シリーズ名: Tables and diagrams for the refrigeration industry = Tables et diagrammes pour l'industrie du froid
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7.

図書

図書
International Institute of Refrigeration
出版情報: Paris : Institut International du Froid, c2001  21 p. ; 30 cm
シリーズ名: Tables and diagrams for the refrigeration industry = Tables et diagrammes pour l'industrie du froid
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8.

図書

図書
International Institute of Refrigeration
出版情報: Paris : Institut International du Froid, c2001  21 p. ; 30 cm
シリーズ名: Tables and diagrams for the refrigeration industry = Tables et diagrammes pour l'industrie du froid
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9.

図書

図書
International Institute of Refrigeration
出版情報: Paris : Institut International du Froid, c2001  23 p. ; 30 cm
シリーズ名: Tables and diagrams for the refrigeration industry = Tables et diagrammes pour l'industrie du froid
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10.

図書

図書
sponsored by IEEE Canada ; edited by Seán Dunne
出版情報: Piscataway, N.J. : Institute of Electrical and Electronics Engineers, c2001  2 v. ; 28 cm
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11.

図書

図書
editors, J. L. van Rooy, C. A. Jermy
出版情報: Pretoria, South Africa : South African Institute of Engineering and Environmental Geologists, c2002  xxiv, 493, 8p. ; 30 cm
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12.

図書

図書
sponsored by IEEE Canada
出版情報: Piscataway, N.J. : Institute of Electrical and Electronics Engineers, c2004  4 v. ; 28 cm
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13.

図書

図書
edited by F. Casoli, J. Lequeux and F. David
出版情報: Berlin : Springer in cooperation with the NATO Scientific Affair Division , Les Ulis : EDP sciences, c2000  xxxiv, 449 p. ; 23 cm
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目次情報: 続きを見る
Lecturers
Participants
Préface
Preface
Contents
Some Quantitative Aspects of Galactic and Extragalactic Infrared Astronomy / M. HarwitCourse 1:
Introduction / 1:
Energy dissipation in cosmic clouds / 2:
Impurities / 3:
Population of excited states / 4:
Cooling rates / 5:
Grains and ices / 6:
Polycyclic aromatic hydrocarbons / 7:
Grain formation / 8:
Cooling of dense clouds by grain radiation / 9:
The Sunyaev-Zel'dovich effect / 10:
The diffuse extragalactic background, cosmic metallicity, and star formation / 11:
Background observations / 12:
Contributions from discrete sources / 13:
Star formation rates, metallicity, and energy production / 14:
Must most of the energy production have occurred at low red shifts z? / 15:
A Single star burnt at red shift z / 15.1:
Continuous formation of massive stars / 15.2:
Low-mass stars / 15.3:
Directly observed star formation / 15.4:
The epoch from which the bulk of the integrated background radiation reaches us / 16:
Overviewof the ISO Mission / M.F. KesslerCourse 2:
ISO satellite
Satellite design / 2.1:
Satellite observing modes / 2.2:
Satellite in-orbit performance / 2.3:
Instrument payload
Overview of instruments / 3.1:
The ISO camera: ISOCAM / 3.2:
The ISO imaging photopolarimeter: ISOPHOT / 3.3:
The ISO short wavelength spectrometer: SWS / 3.4:
The ISO long wavelength spectrometer: LWS / 3.5:
Orbit
Operations
Operations design / 5.1:
Observing time / 5.2:
Operations performance / 5.3:
Scientific highlights
The ISO legacy
ISO data in general / 7.1:
The ISO data archive / 7.2:
Using the ISO data archive / 7.3:
Software tools and overall documentation / 7.4:
Plans until end 2001 / 7.5:
Conclusions
Data Analysis with ISOCAM / J.L. StarkCourse 3:
ISOCAM data calibration
Cosmic ray impact suppression
Dark subtraction for the LW channel
Flat field correction
Stabilization / 2.4:
Jitter / 2.5:
Field of view distortion correction / 2.6:
Source detection in ISOCAM images
Source detection from the wavelet transform
ISOCAM faint source detection: The PRETI method
Calibration from pattern recognition / 3.3.1:
Example / 3.3.3:
Image restoration using the wavelet transform
Image filtering / 4.1:
Image deconvolution / 4.2:
Conclusion
ISO Observations of Solar-System Objects / T. EncrenazCourse 4:
Mars
Giant planets
The D/H ratio
The stratospheres of the giant planets
External source of oxygen in the giant planets / 3.2.1:
Detection of stratospheric hydrocarbons / 3.2.2:
Fluorescence emissions in the stratospheres of Jupiter and Saturn / 3.2.3:
The tropospheres of the giant planets
The 2.7 ?m window
The 7-11 ?m spectrum of Jupiter and Saturn
The far-infrared spectrum of Saturn
The 5-?m spectral window / 3.3.4:
Pluto
Titan
Galilean satellites
Comet Hale-Bopp (C/1995 O1)
Short-period comets
Cometary trails
Distant comets and Kuiper-Belt objects
Asteroids
Zodiacal light
Conclusions and perspectives
Stars and Galactic Structure / H. HabingCourse 5:
The complex objects called stars: Well known and still puzzling
Outline of these notes / 1.1:
Red and Brown dwarfs: Stars of very low mass
Calculations of the structure of M-dwarfs and brown giants
How they look like: Spectra of red and brown dwarfs
The search for red and brown dwarfs: Strategies and results
Luminosity function
Main-sequence stars: Debris disks and planets
The "Vega-effect"
The discovery of planets
Remnant disks as observed by ISO
Red giants
Basic properties of red giants: RGB and AGB stars and later episodes
Recent calculations of stellar structure and stellar evolution
Ab-initio models of the evolution of AGB stars taking mass loss intoaccount / 4.3:
"Synthetic" models of the evolution of AGB stars taking mass lossintoaccount / 4.4:
And what about double stars? / 4.5:
The impact of new observations, especially, but not exclusively, by ISO / 4.6:
AGB stars in our Milky Way and in the Magellanic Clouds
Concluding remarks
Star Formation / A. NattaCourse 6:
Collapse of molecular cores
Giant molecular clouds and cores
Conditions for collapse
Free-fall collapse
Cloud collapse / 2.3.1:
Free-fall accretion / 2.3.2:
Collapse of an isothermal sphere of gas
Collapse of a slowly rotating core
Observable properties of protostars
Evidence of infall from molecular line profiles
SEDs of protostars
The line spectrum of a protostar
Protostellar and pre-main-sequence evolution
The protostellar phase
Pre-main-sequence evolution
The birthline
Circumstellar disks
Accretion disks
Properties of steady accretion disks
The velocity field / 5.2.1:
Timescales / 5.2.2:
Temperature profile and luminosity / 5.2.3:
Density structure / 5.2.4:
Reprocessing disks
Disk-star interaction / 5.4:
SEDs of disks
Power-law disks / 6.1:
Long-wavelength flux and disk mass / 6.2:
Comparison with TTS observations: Heating mechanism / 6.3:
Flared disks / 6.3.1:
Heating by halos / 6.3.2:
Disk atmospheres / 6.3.3:
Disk properties from observations
Mass accretion rate
Inner radius
Masses
Sizes
Disk lifetimes
Ground-based near and mid-infrared surveys / 8.1:
Mid-infrared ISOCAM surveys / 8.2:
ISOPHOT 60 ?m survey / 8.3:
Surveys at millimeter wavelengths / 8.4:
Disk evolution
Can we observe the early planet formation phase? / 9.1:
Evidence for grain growth / 9.2:
Evidence of planetesimals / 9.3:
Where is the disk mass? / 9.4:
Secondary or debris disks
Summary
Dust in the Interstellar Medium / by F. Boulanger ; P. Cox ; A.P. JonesCourse 7:
The phases of the interstellar medium
Abundances
Extinction curve
Infrared emission from dust
Spectral energy distribution
Grain temperatures and infrared emission
Dust composition as a function of size
Interstellar PAHs
Small aromatic hydrocarbons in cirrus / 6.1.1:
Excitation by stellar light / 6.1.2:
Carbon abundance in PAHs / 6.1.3:
Band profiles / 6.1.4:
Very small grains
Large grains
Dust processing in the interstellar medium
Grain sputtering and shattering in shock waves
Physical processes / 7.1.1:
Observations / 7.1.2:
Grain growth in molecular clouds
Dust evolution in clouds / 7.2.1:
Dust evolution in photo-dissociation regions / 7.2.3:
Dense media around protostars
Absorption spectroscopy of embedded sources
Dust around young stars
Dust formation
AGB stars
Infrared spectroscopy of AGB and post-AGB stars
Carbon-rich sources / 9.3.1:
Oxygen-rich sources / 9.3.2:
Evolved planetary nebulae / 9.3.3:
Dust in SNR and hot stars
The life cycle of dust
Sources of dust / 10.1:
The crystalline-amorphous-crystalline silicate transition / 10.2:
Interstellar dust in the solar system / 10.4:
Summary and perspectives
Normal Galaxies in the Infrared / by G. HelouCourse 8:
The study of normal galaxies
Galaxies in the infrared: The IRAS ERA
Basic parameters and statitics
Infrared luminosity / 3.1.1:
The infrared-to-blue ratio / 3.1.2:
IRAS colors / 3.1.3:
Other estimators / 3.1.4:
Correlations
The infrared-radio connection
The "two-component model"
ISO reshapes the dust continuum
ISO surveys of galaxies
Mid-infrared spectra
The aromatic features / 4.2.1:
The mid-infrared continuum / 4.2.2:
High-redshift applications / 4.2.3:
Exceptions / 4.2.4:
The ISO-IRAS color diagram
The global infrared spectrum / 4.3.1:
A mid-infrared look within galaxies
A walk in the line forest
Molecular lines
Fine-structure lines
Interpreting the PDR lines
More studies
Tomorrow's infrared galaxies
Challenges and prospects
Suggestions
Active Galaxies / by D. KunzeCourse 9:
Starburst galaxies
Scales of star formation: From H II regions to starburst galaxies
Observational properties of starburst galaxies
ISO observations of starburst galaxies
The galactic center
Active galactic nuclei
A unified model for AGNs
Massive central black holes
Lecturers
Participants
Préface
14.

図書

図書
edited by P. Binétruy ... [et al.]
出版情報: Les Ulis : EDP sciences , Berlin : Springer, c2000  xxxvi, 628 p. ; 23 cm
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15.

図書

図書
éditeurs
出版情報: Montréal, Québec : Canadian Society for Civil Engineering, c2002  1 v. ; 22 cm
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16.

図書

図書
sponsored by International Gas Union (IGU), International Institute of Refrigeratin (IIR), Institute of Gas Technology (IGT)
出版情報: Des Plaines, Ill. : Gas Technology Institute, c2001  2 v. ; 23 cm
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17.

図書

図書
editors, Guy Olivier, Samuel Pierre, Vijay K. Sood
出版情報: Piscataway, N.J. : Institute of Electrical and Electronics Engineers, c2003  3 v. (xvi, 2086 p.) ; 28 cm
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18.

図書

図書
editor
出版情報: Montréal, Québec : Canadian Society for Civil Engineering, c2003  xxxiii, 260 p. ; 22 cm
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19.

図書

図書
edited by Jean-Louis Barrat ... [et al.] ; published in cooperation with the NATO Scientific Affair Division
出版情報: Les Ulis : EDP Sciences , Berlin ; Tokyo : Springer, c2003  xxxiii, 769 p. ; 23 cm
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20.

図書

図書
edited by H. Flyvbjerg ... [et al.]
出版情報: Les Ulis : EDP sciences , Berlin ; Tokyo : Springer, c2002  xxxiv, 580 p. ; 23 cm
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