Molecules in the stellar environment : proceedings of IAU colloquium No. 146 held at Copenhagen, Denmark, May 24 29, 1993
This volume gives and excellent survey of our present knowledge of molecularprocesses in stellar and proto-stellar objects. It reviews molecular physicsin stellar environments and is intended to bridge the gap between astrophysicists and chemists. The topics range from the theoretical to the computa...
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| المؤلف الرئيسي: | |
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| مؤلف مشترك: | |
| التنسيق: | Livre numérique |
| اللغة: | Anglais |
| منشور في: |
Berlin [etc.] :
Springer
[20..].
Cham : Springer Nature |
| سلاسل: | Lecture notes in physics
428 |
| الموضوعات: | |
| الوصول للمادة أونلاين: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| ملاحظة: |
Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • Molecules in the stellar environment, proceedings of IAU colloquium, n˚146, held at Copenhagen, Denmark, May 24-29, 1993, ed. U. G. Jørgensen, Berlin, Springer-Verlag, 1994, 1 vol. (VIII-440 p.), Lecture notes in physics, 3-540-57747-5 • Molecules in the Stellar Environment, Texte imprimé, 9783662139752 • Molecules in the Stellar Environment, Texte imprimé, 9783662139769 |
جدول المحتويات:
- Stellar photospheres and molecules A view from the bridge
- Dominating molecules in the photospheres of cool stars
- Opacity problems in cool low mass stars
- Molecular opacities in cool dwarf stars
- White dwarfs
- Astrophysical applications of approximate methods for molecular opacities from stars to substellar brown dwarfs
- Infrared spectroscopy and molecules in circumstellar envelopes
- Molecular abundances in the envelopes around evolved stars
- Polvynes and polycyclic aromatic molecules in c-rich circumstellar envelopes
- Improvements in the computation of grain opacity
- From molecules to grains
- Opacity problems in protostellar objects
- Molecules in the sun and molecular data
- Pressure-induced molecular absorption in stellar atmospheres
- Continuous molecular opacities and photodissociation
- Effects of non-local thermodynamic equilibrium (NLTE) on molecular opacities
- Dissociation energies and partition functions of small molecules
- Atomic opacities
- Computation of the absorption coefficient for diatomic molecules
- Computation of opacities for diatomic molecules
- Computation of frequencies and linestrengths for triatomic molecules of astronomical interest
- Computational approaches to determining accurate band strengths
- Ab initio calculations of absorption coefficients of small carbon hydride molecules
- The RASSCF, RASSI, and CASPT2 methods used on small molecules of astrophysical interest
- The MORBID method
- Experimental measurement of weak band intensities
- Oscillator strengths and excited state lifetimes in metallic hydrides and oxides
- The berkeley program on molecules of astrophysical interest
- Production, detection and study in the infrared of unstable molecules and radicals
- Laboratory millimeter wave spectroscopy of smallreactive species
- Table of contents for Poster session proceedings of IAU Colloquium 146: Molecular opacities in the stellar environment .