Abstract Using data from the Wide Field Camera EUV all-sky survey, we have established upper limits to the EUV flux from a sample of 30 bright, nearby, non-active spiral galaxies. These galaxies were chosen to be those most likely to be detected in the EUV on the basis of (i) low interstellar absorption within our own galaxy, (ii) brightness in other wavebands, (iii) high star formation activity, and (iv) proximity. The derived EUV upper limits are restrictive, and establish for the first time that the EUV flux escaping from galaxies does not constitute a major component of their bolometric luminosity, and in particular that it cannot be the sink for the energy injected into the interstellar medium by supernova explosions, as had been suggested following the failure to detect this power in the X-ray band.


    Zugriff

    Zugriff prüfen

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

    EUV emission from normal galaxies


    Beteiligte:
    Ponman, T.J. (Autor:in) / Read, A.M. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 13 , 12 ; 361-364


    Erscheinungsdatum :

    1993-01-01


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



    EUV Emission from Normal Galaxies

    Ponman, T. J. / Read, A. M. / COSPAR | British Library Conference Proceedings | 1993


    EUV Emission from Normal Galaxies

    Ponman, T.J. | Online Contents | 1993



    Dust emission from Lyman-break galaxies

    Takeuchi, Tsutomu T. / Ishii, Takako T. | Elsevier | 2005


    Dust emission from Lyman-break galaxies

    Takeuchi, T. T. / Ishii, T. T. / Committee on Space Research | British Library Conference Proceedings | 2005