Veeresh singh (7 résultats)

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  • Langue : anglais

    Edité par LAP LAMBERT Academic Publishing, 2011

    3846531731 / 9783846531730

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    Vendeur : preigu, Osnabrück, Allemagnepreigu

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    EUR 66,50

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    Taschenbuch. Etat : Neu. Multiwavelength Study of Seyfert Galaxies | Testing the predictions of unification scheme | Veeresh Singh | Taschenbuch | 288 S. | Englisch | 2011 | LAP LAMBERT Academic Publishing | EAN 9783846531730 | Verantwortliche Person für die EU: preigu GmbH & Co. KG, Lengericher Landstr. 19, 49078 Osnabrück, mail[at]preigu[dot]de | Anbieter: preigu.…

  • Langue : anglais

    Edité par Lap Lambert Academic Publishing, 2011

    3846531731 / 9783846531730

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    Vendeur : Revaluation Books, Exeter, Royaume-UniRevaluation Books

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    EUR 164,11

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    Quantité disponible : 1 disponible

    Paperback. Etat : Brand New. 288 pages. 8.66x5.91x0.65 inches. In Stock.

  • Langue : anglais

    Edité par LAP LAMBERT Academic Publishing, 2011

    3846531731 / 9783846531730

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    Vendeur : Mispah books, Redhill, SURRE, Royaume-UniMispah books

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    EUR 251,13

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    paperback. Etat : New. NEW. SHIPS FROM MULTIPLE LOCATIONS. book.

  • Langue : anglais

    Edité par LAP LAMBERT Academic Publishing Nov 2011, 2011

    3846531731 / 9783846531730

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    Vendeur : BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, AllemagneBuchWeltWeit Ludwig Meier e.K.

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    EUR 79,00

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    Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Seyfert galaxies are a subclass of active galaxies and are categorized as nearby, low luminosity, radio-quiet Active Galactic Nuclei (AGN) hosted in spiral or lenticular galaxies. Seyfert galaxies are classified mainly into two subclasses named as `type 1' and `type 2' based on the presence and absence of broad permitted emission lines in their optical spectra, respectively. Seyfert unification scheme hypothesizes that Seyfert type 1s and type 2s belong to the same parent population and appear different solely due to the differing orientations of the obscuring material having a torus-like geometry around the AGN. The primary objective of this work is to examine the validity and limitations of the orientation and obscuration based Seyfert unification scheme using multiwavelength (mainly X-ray and radio) observations. It has been emphasized that the key issue in testing the Seyfert unification scheme is acquiring a well defined Seyfert sample. The statistical comparisons of X-ray, radio and IR properties of the two Seyfert subtypes have been discussed in the framework of the unification scheme. 288 pp. Englisch.…

  • Langue : anglais

    Edité par LAP LAMBERT Academic Publishing, 2011

    3846531731 / 9783846531730

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    Vendeur : moluna, Greven, Allemagnemoluna

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    EUR 63,42

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    Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: Singh VeereshDr. Veeresh Singh obtained Ph.D. in Physics from Indian Institute of Astrophysics, Bangalore. His research interests cover phenomenological study of Active Galactic Nuclei, unification models of AGNs, star formation and .…

  • Langue : anglais

    Edité par LAP LAMBERT Academic Publishing, 2011

    3846531731 / 9783846531730

    • Couverture souple
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    Vendeur : AHA-BUCH GmbH, Einbeck, AllemagneAHA-BUCH GmbH

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    EUR 79,00

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    Taschenbuch. Etat : Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - Seyfert galaxies are a subclass of active galaxies and are categorized as nearby, low luminosity, radio-quiet Active Galactic Nuclei (AGN) hosted in spiral or lenticular galaxies. Seyfert galaxies are classified mainly into two subclasses named as `type 1' and `type 2' based on the presence and absence of broad permitted emission lines in their optical spectra, respectively. Seyfert unification scheme hypothesizes that Seyfert type 1s and type 2s belong to the same parent population and appear different solely due to the differing orientations of the obscuring material having a torus-like geometry around the AGN. The primary objective of this work is to examine the validity and limitations of the orientation and obscuration based Seyfert unification scheme using multiwavelength (mainly X-ray and radio) observations. It has been emphasized that the key issue in testing the Seyfert unification scheme is acquiring a well defined Seyfert sample. The statistical comparisons of X-ray, radio and IR properties of the two Seyfert subtypes have been discussed in the framework of the unification scheme.…

  • Langue : anglais

    Edité par LAP LAMBERT Academic Publishing Nov 2011, 2011

    3846531731 / 9783846531730

    • Couverture souple
    • impression à la demande

    Vendeur : buchversandmimpf2000, Emtmannsberg, BAYE, Allemagnebuchversandmimpf2000

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    EUR 79,00

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    Quantité disponible : 1 disponible

    Taschenbuch. Etat : Neu. This item is printed on demand - Print on Demand Titel. Neuware -Seyfert galaxies are a subclass of active galaxies and are categorized as nearby, low luminosity, radio-quiet Active Galactic Nuclei (AGN) hosted in spiral or lenticular galaxies. Seyfert galaxies are classified mainly into two subclasses named as `type 1' and `type 2' based on the presence and absence of broad permitted emission lines in their optical spectra, respectively. Seyfert unification scheme hypothesizes that Seyfert type 1s and type 2s belong to the same parent population and appear different solely due to the differing orientations of the obscuring material having a torus-like geometry around the AGN. The primary objective of this work is to examine the validity and limitations of the orientation and obscuration based Seyfert unification scheme using multiwavelength (mainly X-ray and radio) observations. It has been emphasized that the key issue in testing the Seyfert unification scheme is acquiring a well defined Seyfert sample. The statistical comparisons of X-ray, radio and IR properties of the two Seyfert subtypes have been discussed in the framework of the unification scheme.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 288 pp. Englisch.…