Articles liés à Infrared Spectra of Astrophysical PAHs: A Density Functional...
Synopsis
The aromatic infrared bands (AIBs) centred at 3.3, 6.2, 7.7, 8.6 and 11.2 microns are ubiquitous in diverse interstellar sources including HII regions, reflection nebulae, planetary nebulae, star forming regions, interstellar medium (ISM) of Milky Way as well as external galaxies. Important differences in spectral details have emerged with quality observational data from space based telescopes ISO and SPITZER. The hypothesis that polycyclic aromatic hydrocarbons (PAHs) are the most viable carriers of AIBs was proposed more than two decades back. The infrared (IR) spectra of PAHs is consistent with characteristic frequencies of the AIBs. Improved laboratory and computational spectroscopic techniques have strengthened the hypothesis and PAHs are now considered as important inhabitants of the ISM incorporating substantial fraction of carbon. Theoretical quantum chemical calculations provide an alternative to obtain the IR information of complex species such as substituted and very large and irregular PAHs. The results of theoretical calculations have been used in IR emission models.
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- ÉditeurLAP LAMBERT Academic Publishing
- Date d'édition2015
- ISBN 10 3659453757
- ISBN 13 9783659453755
- ReliureBroché
- Langueanglais
- Nombre de pages232
- Coordonnées du fabricantnon disponible
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Infrared Spectra of Astrophysical PAHs
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LAP LAMBERT Academic Publishing, 2015
ISBN 10 : 3659453757
ISBN 13 : 9783659453755
Neuf
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Vendeur : moluna, Greven, Allemagne
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Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: Pathak AmitAmit Pathak completed his PhD in Physics from Gorakhpur University in the year 2006. His work was on theoretically simulating the vibrational spectra of large aromatic molecules that are a significant constituent of the in. N° de réf. du vendeur 21509063
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Infrared Spectra of Astrophysical PAHs
Edité par
LAP LAMBERT Academic Publishing Mrz 2015, 2015
ISBN 10 : 3659453757
ISBN 13 : 9783659453755
Neuf
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Vendeur : BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Allemagne
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Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The aromatic infrared bands (AIBs) centred at 3.3, 6.2, 7.7, 8.6 and 11.2 microns are ubiquitous in diverse interstellar sources including HII regions, reflection nebulae, planetary nebulae, star forming regions, interstellar medium (ISM) of Milky Way as well as external galaxies. Important differences in spectral details have emerged with quality observational data from space based telescopes ISO and SPITZER. The hypothesis that polycyclic aromatic hydrocarbons (PAHs) are the most viable carriers of AIBs was proposed more than two decades back. The infrared (IR) spectra of PAHs is consistent with characteristic frequencies of the AIBs. Improved laboratory and computational spectroscopic techniques have strengthened the hypothesis and PAHs are now considered as important inhabitants of the ISM incorporating substantial fraction of carbon. Theoretical quantum chemical calculations provide an alternative to obtain the IR information of complex species such as substituted and very large and irregular PAHs. The results of theoretical calculations have been used in IR emission models. 232 pp. Englisch. N° de réf. du vendeur 9783659453755
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Infrared Spectra of Astrophysical PAHs : A Density Functional Theory Approach
Edité par
LAP LAMBERT Academic Publishing, 2015
ISBN 10 : 3659453757
ISBN 13 : 9783659453755
Neuf
Taschenbuch
Vendeur : AHA-BUCH GmbH, Einbeck, Allemagne
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Taschenbuch. Etat : Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - The aromatic infrared bands (AIBs) centred at 3.3, 6.2, 7.7, 8.6 and 11.2 microns are ubiquitous in diverse interstellar sources including HII regions, reflection nebulae, planetary nebulae, star forming regions, interstellar medium (ISM) of Milky Way as well as external galaxies. Important differences in spectral details have emerged with quality observational data from space based telescopes ISO and SPITZER. The hypothesis that polycyclic aromatic hydrocarbons (PAHs) are the most viable carriers of AIBs was proposed more than two decades back. The infrared (IR) spectra of PAHs is consistent with characteristic frequencies of the AIBs. Improved laboratory and computational spectroscopic techniques have strengthened the hypothesis and PAHs are now considered as important inhabitants of the ISM incorporating substantial fraction of carbon. Theoretical quantum chemical calculations provide an alternative to obtain the IR information of complex species such as substituted and very large and irregular PAHs. The results of theoretical calculations have been used in IR emission models. N° de réf. du vendeur 9783659453755
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Infrared Spectra of Astrophysical PAHs
Edité par
LAP LAMBERT Academic Publishing Mär 2015, 2015
ISBN 10 : 3659453757
ISBN 13 : 9783659453755
Neuf
Taschenbuch
Vendeur : buchversandmimpf2000, Emtmannsberg, BAYE, Allemagne
Évaluation du vendeur 5 sur 5 étoiles
Taschenbuch. Etat : Neu. This item is printed on demand - Print on Demand Titel. Neuware -The aromatic infrared bands (AIBs) centred at 3.3, 6.2, 7.7, 8.6 and 11.2 microns are ubiquitous in diverse interstellar sources including HII regions, reflection nebulae, planetary nebulae, star forming regions, interstellar medium (ISM) of Milky Way as well as external galaxies. Important differences in spectral details have emerged with quality observational data from space based telescopes ISO and SPITZER. The hypothesis that polycyclic aromatic hydrocarbons (PAHs) are the most viable carriers of AIBs was proposed more than two decades back. The infrared (IR) spectra of PAHs is consistent with characteristic frequencies of the AIBs. Improved laboratory and computational spectroscopic techniques have strengthened the hypothesis and PAHs are now considered as important inhabitants of the ISM incorporating substantial fraction of carbon. Theoretical quantum chemical calculations provide an alternative to obtain the IR information of complex species such as substituted and very large and irregular PAHs. The results of theoretical calculations have been used in IR emission models.Books on Demand GmbH, Überseering 33, 22297 Hamburg 232 pp. Englisch. N° de réf. du vendeur 9783659453755
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