Deutsch
 
Hilfe Datenschutzhinweis Impressum
  DetailsucheBrowse

Datensatz

DATENSATZ AKTIONENEXPORT
Zur Ablage hinzufügen
 Lokale TagsFreigabegeschichteDetailsÜbersicht
  Electron-Ion Recombination Measurements Motivated by AGN X-Ray Absorption Features: Fe XIV Forming Fe XIII

Schmidt, E., Schippers, S., Mueller, A., Lestinsky, M., Sprenger, F., Grieser, M., et al. (2006). Electron-Ion Recombination Measurements Motivated by AGN X-Ray Absorption Features: Fe XIV Forming Fe XIII. The Astrophysical Journal, 641(2, part 2), L157-L160.

Item is

 

einblenden: alle ausblenden: alle

Basisdaten

einblenden: ausblenden:
Datensatz-Permalink: https://hdl.handle.net/11858/00-001M-0000-0011-804F-0 Versions-Permalink: https://hdl.handle.net/11858/00-001M-0000-0011-8050-A
Genre: Zeitschriftenartikel

Externe Referenzen

einblenden:

Urheber

einblenden:
ausblenden:
 Urheber:
Schmidt, E.W.1, Autor
Schippers, S.2, Autor           
Mueller, A.1, Autor
Lestinsky, M.2, Autor           
Sprenger, F.2, Autor           
Grieser, M.2, Autor           
Repnow, R.2, Autor           
Wolf, A.2, Autor           
Brandau, C.1, Autor
Lukic, D.1, Autor
Schnell, M.3, Autor           
Savin, D.W.1, Autor
Affiliations:
1Institut für Atom- und Molekülphysik, Justus-Liebig-Universität, Leihgesterner Weg 217, D-35392 Giessen, Germany. Gesellschaft für Schwerionenforschung, Planckstrasse 1, D-64291 Darmstadt, Germany. Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027., ou_persistent22              
2Division Prof. Dr. Klaus Blaum, MPI for Nuclear Physics, Max Planck Society, ou_904548              
3Prof. Dirk Schwalm, Emeriti, MPI for Nuclear Physics, Max Planck Society, ou_907546              

Inhalt

einblenden:
ausblenden:
Schlagwörter: -
 Zusammenfassung: Recent spectroscopic models of active galactic nuclei (AGNs) have indicated that the recommended electron-ion recombination rate coefficients for iron ions with partially filled M shells are incorrect in the temperature range where these ions form in photoionized plasmas. We have investigated this experimentally for Fe XIV forming Fe XIII. The recombination rate coefficient was measured by employing the electron-ion merged-beams method at the Heidelberg heavy-ion test storage ring. The measured energy range of 0-260 eV encompasses all dielectronic recombination 1s22s22p63l3l3l nl resonances associated with the 3p1/2 3p3/2, 3s 3p, 3p 3d, and 3s 3d core excitations within the M shell of the Fe XIV (1s22s22p63s23p) parent ion. This range also includes the 1s22s22p63l3l4l nl resonances associated with 3s 4l and 3p 4l core excitations. We find that in the temperature range 2-14 eV, where Fe XIV is expected to form in a photoionized plasma, the Fe XIV recombination rate coefficient is orders of magnitude larger than previously calculated values.

Details

einblenden:
ausblenden:
Sprache(n): eng - English
 Datum: 2006-04
 Publikationsstatus: Erschienen
 Seiten: -
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
 Art der Begutachtung: Expertenbegutachtung
 Identifikatoren: eDoc: 281370
 Art des Abschluß: -

Veranstaltung

einblenden:

Entscheidung

einblenden:

Projektinformation

einblenden:

Quelle 1

einblenden:
ausblenden:
Titel: The Astrophysical Journal
Genre der Quelle: Zeitschrift
 Urheber:
Affiliations:
Ort, Verlag, Ausgabe: -
Seiten: - Band / Heft: 641 (2, part 2) Artikelnummer: - Start- / Endseite: L157 - L160 Identifikator: -