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  • 1
    UID:
    b3kat_BV041964131
    Umfang: 1 Online-Ressource
    ISBN: 9783540577478
    Serie: Lecture notes in physics 428
    Weitere Ausg.: Erscheint auch als Druckausgabe ISBN 978-3-540-48327-4
    Sprache: Englisch
    Schlagwort(e): Sternatmosphäre ; Molekül ; Molekülspektroskopie ; Stern ; Sternentwicklung ; Interstellare Materie ; Konferenzschrift
    Bibliothek Standort Signatur Band/Heft/Jahr Verfügbarkeit
    BibTip Andere fanden auch interessant ...
  • 2
    UID:
    gbv_749240539
    Umfang: 1 Online-Ressource (VIII, 444 p. 25 illus)
    Ausgabe: Springer eBook Collection. Physics and Astronomy
    ISBN: 9783540483274 , 9783540577478
    Serie: Lecture Notes in Physics 428
    Inhalt: 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 computational and include observational data. Among the topics treated are questions of stellar evolution, the determination of physical propertiesand structures , and the chemical composition of stellar protospheres. Opacity is studied in the context of various types of stellar and proto-stellar objects
    Inhalt: 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 small reactive species -- Table of contents for “Poster session proceedings of IAU Colloquium 146: Molecular opacities in the stellar environment”
    Weitere Ausg.: ISBN 9783540577478
    Sprache: Englisch
    Bibliothek Standort Signatur Band/Heft/Jahr Verfügbarkeit
    BibTip Andere fanden auch interessant ...
  • 3
    UID:
    almahu_9947923361002882
    Umfang: VIII, 444 p. 25 illus. , online resource.
    ISBN: 9783540483274
    Serie: Lecture Notes in Physics, 428
    Inhalt: 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 computational and include observational data. Among the topics treated are questions of stellar evolution, the determination of physical propertiesand structures , and the chemical composition of stellar protospheres. Opacity is studied in the context of various types of stellar and proto-stellar objects.
    Anmerkung: 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 small reactive species -- Table of contents for “Poster session proceedings of IAU Colloquium 146: Molecular opacities in the stellar environment”.
    In: Springer eBooks
    Weitere Ausg.: Printed edition: ISBN 9783540577478
    Sprache: Englisch
    Bibliothek Standort Signatur Band/Heft/Jahr Verfügbarkeit
    BibTip Andere fanden auch interessant ...
  • 4
    Online-Ressource
    Online-Ressource
    Berlin, Heidelberg :Springer Berlin Heidelberg :
    UID:
    edocfu_9959186125102883
    Umfang: 1 online resource (VIII, 444 p. 25 illus.)
    Ausgabe: 1st ed. 1994.
    Ausgabe: Online edition Springer Lecture Notes Archive ; 041142-5
    ISBN: 3-540-48327-6
    Serie: Lecture Notes in Physics, 428
    Inhalt: 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 computational and include observational data. Among the topics treated are questions of stellar evolution, the determination of physical propertiesand structures , and the chemical composition of stellar protospheres. Opacity is studied in the context of various types of stellar and proto-stellar objects.
    Anmerkung: 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 small reactive species -- Table of contents for “Poster session proceedings of IAU Colloquium 146: Molecular opacities in the stellar environment”.
    In: Springer eBooks
    Weitere Ausg.: ISBN 3-540-57747-5
    Sprache: Englisch
    Bibliothek Standort Signatur Band/Heft/Jahr Verfügbarkeit
    BibTip Andere fanden auch interessant ...
  • 5
    Online-Ressource
    Online-Ressource
    Berlin, Heidelberg :Springer Berlin Heidelberg :
    UID:
    edoccha_9959186125102883
    Umfang: 1 online resource (VIII, 444 p. 25 illus.)
    Ausgabe: 1st ed. 1994.
    Ausgabe: Online edition Springer Lecture Notes Archive ; 041142-5
    ISBN: 3-540-48327-6
    Serie: Lecture Notes in Physics, 428
    Inhalt: 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 computational and include observational data. Among the topics treated are questions of stellar evolution, the determination of physical propertiesand structures , and the chemical composition of stellar protospheres. Opacity is studied in the context of various types of stellar and proto-stellar objects.
    Anmerkung: 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 small reactive species -- Table of contents for “Poster session proceedings of IAU Colloquium 146: Molecular opacities in the stellar environment”.
    In: Springer eBooks
    Weitere Ausg.: ISBN 3-540-57747-5
    Sprache: Englisch
    Bibliothek Standort Signatur Band/Heft/Jahr Verfügbarkeit
    BibTip Andere fanden auch interessant ...
  • 6
    Online-Ressource
    Online-Ressource
    Berlin, Heidelberg :Springer Berlin Heidelberg :
    UID:
    almafu_9959186125102883
    Umfang: 1 online resource (VIII, 444 p. 25 illus.)
    Ausgabe: 1st ed. 1994.
    Ausgabe: Online edition Springer Lecture Notes Archive ; 041142-5
    ISBN: 3-540-48327-6
    Serie: Lecture Notes in Physics, 428
    Inhalt: 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 computational and include observational data. Among the topics treated are questions of stellar evolution, the determination of physical propertiesand structures , and the chemical composition of stellar protospheres. Opacity is studied in the context of various types of stellar and proto-stellar objects.
    Anmerkung: 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 small reactive species -- Table of contents for “Poster session proceedings of IAU Colloquium 146: Molecular opacities in the stellar environment”.
    In: Springer eBooks
    Weitere Ausg.: ISBN 3-540-57747-5
    Sprache: Englisch
    Bibliothek Standort Signatur Band/Heft/Jahr Verfügbarkeit
    BibTip Andere fanden auch interessant ...
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