Galactic abundances: Report of working group 3
| Autor: | Berndt Klecker, John) Martin Laming, E. O. Flückiger, H. Kunow, F. Buclin, A. C. Cummings, U. J. Sofia, K.-P. Wenzel, J. W. Keller, Friedrich-Karl Thielemann, J. S. George, E. Salerno, M. Y. Hofer, E. C. Stone, C. Tranquille, D. Kirilova, E. R. Christian, M. E. Wiedenbeck, Volker Bothmer, Frank C. Jones |
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| Přispěvatelé: | Wimmer-Schweingruber, R. F. |
| Rok vydání: | 2001 |
| Předmět: |
Physics
Solar System Astrophysics::High Energy Astrophysical Phenomena Young stellar object Astronomy Context (language use) Cosmic ray Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics Galaxy Spectral line Interstellar medium Meteorite Astrophysics::Solar and Stellar Astrophysics Astrophysics::Galaxy Astrophysics |
| Zdroj: | AIP Conference Proceedings. |
| ISSN: | 0094-243X |
| DOI: | 10.1063/1.1434002 |
| Popis: | We summarize the various methods and their limitations and strengths to derive galactic abundances from in-situ and remote-sensing measurements, both from ground-based observations and from instruments in space. Because galactic abundances evolve in time and space it is important to obtain information with a variety of different methods covering different regions from the Very Local Insterstellar Medium (VLISM) to the distant galaxy, and different times throughout the evolution of the galaxy. We discuss the study of the present-day VLISM with neutral gas, pickup ions, and Anomalous Cosmic Rays, the study of the local interstellar medium (ISM) at distances |
| Databáze: | OpenAIRE |
| Externí odkaz: |
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