Dusty Objects in the Universe Proceedings of the Fourth International Workshop of the Astronomical Observatory of Capodimonte (OAC 4), Held at Capri, Italy, September 8–13, 1989
Solid matter in space is crucial in accounting for many processes. In these last years a great improvement of the general knowledge of the problem has been possible due to the increase, in number and quality, of observations and of the laboratory efforts to simulate "cosmic" dust. Theoreti...
| Other Authors: | , |
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| Format: | eBook |
| Language: | English |
| Published: |
Dordrecht
Springer Netherlands
1990, 1990
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| Edition: | 1st ed. 1990 |
| Series: | Astrophysics and Space Science Library
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| Subjects: | |
| Online Access: | |
| Collection: | Springer Book Archives -2004 - Collection details see MPG.ReNa |
Table of Contents:
- Proceedings
- Carbonaceous Solid Materials: From Laboratory to Space
- Chemical Alterations in Ion Irradiated Frozen Hydrocarbons
- Investigation of Cosmic Dusts Using Synchrotron Radiation
- The Particles Around Mass-Losing Carbon Stars
- The Infrared Interstellar Emission Features
- Quenced Carbonaceous Composite (QCC): Thermal Alteration of QCC and PAHs
- Mineral Grains in Interstellar Space
- Novel Ion Chemistry of Interstellar Polycyclic Aromatic Hydrocarbons
- Astrophysical Implications of the Infrared Spectrum of Coronene at Elevated Temperatures
- The 3.3 Micrometer Feature: The Large Scale Galactic Emission
- Search for the UV and IR Spectra of C6 0 in Laboratory-Produced Carbon Dust
- Circumstellar Dust Envelopes of M Giant Stars
- Interstellar Planetesimals
- The Anatomy of Dense Molecular Clouds
- S O F I A — A Stratospheric Observatory for Infrared Astronomy
- Observations of the Cold Dust and Gas in Centaurus A: Probing an Extragalactic ISM
- Extragalactic Extinction: The Optical Data for the Early-Type Galaxy NGC 2534
- Possible Existence of Dust in Nearby Galaxy Group
- Interaction of Dust Particles with Electrons and Ions
- Are Spiral Galaxies Optically Thick?
- On the Possible Interaction between Magnetic Field and HII Region in AB Aur
- A Model of the Cometary Dust Trails Detected by IRAS
- The Dust Tail of Comet Bradfield 1987XXIX
- The Dust Properties of High-Mass Star-Forming Regions
- On the Energetic Component of FU Ori Wind
- Models for Infrared Emission from Galaxies
- Elliptical Galaxies with Dust Lanes
- Observational Cosmology in the Near Infra-Red
- Intracluster Extinction of Light from Galaxies in Virgo
- Axially Symmetric Radiative Transfer Models of Low Mass Protostars
- The Infrared Space Observatory (ISO)
- Modulation at 10 µm with Array Detectors?
- Posters
- Near-Infrared Spectra of the Extended Young Objects GL 2591 and NGC 7538/IRS9
- The 3.3 µm Feature,H2, and Ionized Gas in the Orion Bar
- The Extended 3.3 µm Emission Feature in the Orion’s Cloud