Structure and dynamics of the interstellar medium : proceedings of IAU Colloquium No. 120, held on the occasion of Guido's Jubilee in Granada, Spain, April 17-21, 1989
Here for the first time is a book that treats practically all aspects of modern research in interstellar matter astrophysics. 20 review articles and 40 carefully selected and refereed papers give a thorough overview of the field and convey the flavor of enthusiastic colloquium discussions to the rea...
Guardat en:
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| Autor corporatiu: | |
| Altres autors: | , |
| Format: | Livre numérique |
| Idioma: | Anglais |
| Publicat: |
Berlin [etc.] :
Springer
[20..].
Cham : Springer Nature |
| Col·lecció: | Lecture notes in physics
350 |
| Matèries: | |
| Accés en línia: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| Nota: |
Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • Structure and Dynamics of the Interstellar Medium, Texte imprimé, 9783540519560 • Structure and Dynamics of the Interstellar Medium, Texte imprimé, 9783662137598 • Structure and Dynamics of the Interstellar Medium, Texte imprimé, 9783662137604 |
Taula de continguts:
- Chemistry of molecular clouds
- CO distributions towards the southern dark cloud of DC 303.6+0.9
- Extensive molecular line survey for dark clouds
- Molecular hydrogen emission from photodissociation regions
- Cosmic ray induced photodestruction of interstellar molecules
- The nature of shocks in molecular clouds
- Fragmentation and the initial mass function
- Star formation
- Turbulence in interstellar clouds
- Turbulent and ordered motions in HII regions
- Expansion of HII regions in density gradients
- Variable HII regions
- The sharpless 187 gas complex: A study of the molecular, atomic, ionized and dust components
- Turbulent mixing in wind-blown HII regions
- Accretion flows in high-mass star formation
- An optical study of the star formation region NGC 7129
- Star formation in the NGC 2071 molecular cloud
- A theory on the slope of the IMF
- S266: A distant HII region in the Galaxy
- Silicon bearing molecules in molecular clouds
- Dense clumps in NGC 2024 Protostellar condensations?
- Radio maps of the regions RCW 57 and W 49
- Ionization of the galactic center arched filaments
- The chamaeleon dark clouds complex: Preliminary analysis of the colour excesses E(b-y) towards the selected Area 203
- Interstellar wind-blown bubbles
- Stellar winds in a-type supergiants
- Supernova remnants
- Dust condensation in the ejecta of SN 1987A
- Observations of the progenitor wind of SN 1987A
- The dynamical evolution of a clumpy medium
- Infrared environment of the be star 6 cephei: Interaction of stellar and interstellar winds
- Carbon monoxide emission from young planetary nebulae
- Interaction between a stellar wind and the ionized gas in N120 (LMC)
- Disks and outflows
- The structure of dense cloud cores
- Molecular disks around young stars
- On the nature of thebeta pictoris circumstellar nebula
- Near-infrared images of the serpens molecular cloud core
- Molecular outflows
- Submillimetre mapping and photometry of bipolar flows Evidence for compact disks
- AFGL 2591 and monoceros R2: Cavities in the molecular cloud
- Aperture synthesis observations of CS. NH3. and continuum in the bipolar flow source NGC2071-IRS
- A swept-up molecular bubble in L1551
- On the formation and propagation of interstellar jets
- The collimation of nonadiabatic winds from young stars
- Herbig-Haro objects
- A CO search for molecular gas in high mass post-main-sequence nebulae
- A remarkable bipolar flow in the center of the Rho ophiuchi cloud
- Massive dust disks surrounding herbig Ae/Be stars
- New young objects from the iras point source catalogue
- IUE observations of herbig-haro objects 7, 11 & 29
- H2 2.12 m spectroscopy and imaging of HH objects
- New OVRO results show disks are not necessary for focussing bipolar outflows
- The spectrum of a partially ionized jet
- Sodium ionization in T-tauri stars
- Inverting the position-velocity diagrams of molecular discs
- Identification of outflow exciting sources through ammonia observations
- The molecular envolope of mira
- Narrowband photometry of photometrically peculiar objects
- The structure of molecular clouds from large scale surveys of CO and CS
- The radio continuum morphology of the Orion Nebula
- Highly excited molecular hydrogen in orion
- Aperture synthesis observations of NH3 and CS in Orion-KL
- The trapezium radio cluster of the Orion Nebula
- Turbulence in the Orion Nebula
- High-resolution molecular line observations of the core and outflow in orion B
- Star formation in galactic nuclei
- Ionized gas and stellar content in a sample of HII galaxies
- The shaping of theoptical jet of the galaxy NGC 4258
- A plasmon driven bowshock model for the narrow line region of NGC5929
- Age effects in Giant Extragalactic HII Regions
- Evolution of clumpy gas in galaxies
- H?-emission in directions toward high velocity 21cm clouds
- High-velocity absorption components toward the LMC
- Distance and chemical composition of high-velocity clouds
- Inflow of neutral gas toward the galactic disk
- Ultraviolet observations of halo clouds
- Analysis of low- and high-resolution observations of high-velocity clouds
- Molecules at the interface of an HVC and a high-z HI filament
- Observations of the galactic halo
- A new high-resolution optical study of halo gas
- Galactic winds
- Cycling of dust grains through the galactic halo
- The intermediate velocity cloud IVC86+38.5-45, related to high velocity clouds?
- The NaI interstellar spectrum of HVC 287.5+225+240
- Collisions between high latitude clouds: Theory meets observations
- Multiple-supernova remnants
- Galactic fountains
- Clustered supernovae vs. the gaseous disk and halo A rematch
- Gamma rays from violent interstellar events
- Structure of the diffuse interstellar medium
- The mass spectrum of interstellar clouds
- Deterministic self-propagating star formation
- The violent interstellar medium in messier 31
- Contributions of supernovae to the chemical and dynamical evolution of the ism
- 1/4 Ke V diffuse background and the local interstellar medium
- Large-scale irregularities in the interstellar medium
- The milky way disk warp.