Atomic and Molecular Data for Space Astronomy Needs, Analysis, and Availability [electronic resource] : A Selection of Papers Presented at the Joint Commission Meeting III of the 21st IAU General Assembly Held in Buenos Aires, Argentina 23 July – 1 August 1991 / edited by Peter L. Smith, Wolfgang L. Wiese.
Material type:
TextSeries: Lecture Notes in Physics ; 407Publisher: New York, NY : Springer New York, 1992Description: VII, 160 p. online resourceContent type: - text
- computer
- online resource
- 9780387348308
- A Selection of Papers Presented at the Joint Commission Meeting III of the 21st IAU General Assembly Held in Buenos Aires, Argentian 23 July - 1 August 1991
- 520 23
- QB4
E-BOOKS
| Home library | Call number | Materials specified | URL | Status | Date due | Barcode | |
|---|---|---|---|---|---|---|---|
| IMSc Library | Link to resource | Available | EBK2043 |
Atomic and molecular data for space astronomy: Needs and availability -- The hubble space telescope — Scientific problems and laboratory data needs -- Atomic data needed for far ultraviolet astronomy with HUT and FUSE -- Atomic data needed for analysis of EUV and X-Ray spectra -- Atomic and molecular data for observations of the interstellar medium with the hubble space telescope -- Atomic and molecular data needed for analysis of infrared spectra from ISO and SIRTF -- Atomic data from the opacity project -- Sources of atomic spectroscopic data for astrophysics -- Summary of current molecular databases.
This is a very useful reference book for working astronomers and astrophysicists. Forming the proceedings of a recent IAU meeting where the availability and the needs of atomic and molecular data were discussed, the papers published here discuss existing and planned instruments for astronomical spectroscopy from earth-orbiting satellites. In particular, the atomic and molecular parameters that are, or will be, needed for analysis of the data obtained by these instruments are considered. A number of significant shortcomings in the available databases are identified. The needs highlighted will be of interest to laboratory astrophysicists, both experimentalists and theorists, who canproduce the data required. A second group of papers provides a current inventory of atomic and molecular data compilations.
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