Astronomie spatiale infrarouge, aujourd'hui et demain : Les Houches, session LXX, 3-28 August 1998 = Infrared space astronomy, today and tomorrow

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Astronomie spatiale infrarouge, aujourd'hui et demain : Les Houches, session LXX, 3-28 August 1998 = Infrared space astronomy, today and tomorrow / edited by F. Casoli, J. Lequeux and F. David

資料種別:

図書

出版情報:

Berlin : Springer in cooperation with the NATO Scientific Affair Division
Les Ulis : EDP sciences, c2000

形態:

xxxiv, 449 p. ; 23 cm

著者名:

ISBN:

9783540673866 [3540673865] (: Springer)
9782868834690 [2868834698] (: EDP sciences)

書誌ID:

BA48370206

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その他の標題:

Infrared space astronomy, today and tomorrow : Les Houches, session LXX, NATO ASI

注記:

At head of title:École de physique des Houches-UJFG & INPG-Grenoble
Includes bibliographical references
"A NATO advanced study institute"

主題:

Infrared astronomy--Congresses

言語:

英語; フランス語

目次情報:

Lecturers

Participants

PrÃ©face

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

PrÃ©face

Preface

Contents

Some Quantitative Aspects of Galactic and Extragalactic Infrared Astronomy / M. HarwitCourse 1：

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