Abstract We have used Far Ultraviolet Spectroscopic Explorer (FUSE) observations of the Large Magellanic Cloud (LMC) to determine the O vi column densities in the Milky Way (MW) towards 6 LMC lines of sight. The mean column density of O vi in the MW is found to be log N(O vi)= 14.257 - 0.084 + 0.096 . The results confirm the patchiness of O vi absorption in the MW and the column densities are higher or comparable to the LMC.


    Zugriff

    Zugriff prüfen

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

    O vi absorption in the Milky Way along the Large Magellanic Cloud lines of sight


    Beteiligte:
    Sarma, Rathin (Autor:in) / Pathak, Amit (Autor:in) / Pradhan, Ananta C. (Autor:in) / Murthy, Jayant (Autor:in) / Sarma, Jayanta K. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 53 , 6 ; 963-966


    Erscheinungsdatum :

    2013-01-01


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch






    Starburst-like Dust in the Small Magellanic Cloud

    Gordon, K. D. / Clayton, G. C. | British Library Online Contents | 1998


    New High Resolution X-ray Studies of Magellanic Cloud Supernova Remnants

    Williams, R. N. M. / Chu, Y.-H. / Chen, C.-H. et al. | British Library Conference Proceedings | 2005


    LIDAR AIR DATA SYSTEM WITH DECOUPLED LINES OF SIGHT

    GRANT LODDEN / MATTHEW WIEBOLD / JASON GARDE | Europäisches Patentamt | 2019

    Freier Zugriff