Sie befinden Sich nicht im Netzwerk der Universität Paderborn. Der Zugriff auf elektronische Ressourcen ist gegebenenfalls nur via VPN oder Shibboleth (DFN-AAI) möglich. mehr Informationen...
Ergebnis 1 von 158

Details

Autor(en) / Beteiligte
Titel
Spectral Energy Distributions of Southern Binary X-Ray Sources
Ist Teil von
  • The Astrophysical journal. Supplement series, 2023-09, Vol.268 (1), p.35
Ort / Verlag
Saskatoon: The American Astronomical Society
Erscheinungsjahr
2023
Quelle
EZB Electronic Journals Library
Beschreibungen/Notizen
  • Abstract The rapid variability of X-ray binaries (XRBs) produces a wide range of X-ray states that are linked to activity across the electromagnetic spectrum. It is particularly challenging to study a sample of sources large enough to include all types in their various states, and to cover the full range of frequencies that show flux density variations. Simultaneous observations with many telescopes are necessary. In this project, we monitor 48 XRBs with seven telescopes across the electromagnetic spectrum from 5 × 10 9 to 10 19 Hz, including ground-based radio, IR, and optical observatories, and five instruments on two spacecraft over a 1 week period. We construct spectral energy distributions and matching X-ray color–intensity diagrams for 20 sources that have the most extensive detections. Our observations are consistent with several models of expected behavior proposed for the different classes: we detect no significant radio emission from pulsars or atoll sources, but we do detect radio emission from Z sources in the normal or horizontal branch, and from black holes in the high/soft, low/hard, and quiescent states. The survey data provide useful constraints for more detailed models predicting behavior from the different classes of sources.
Sprache
Englisch
Identifikatoren
ISSN: 0067-0049
eISSN: 1538-4365
DOI: 10.3847/1538-4365/ace4b9
Titel-ID: cdi_iop_journals_10_3847_1538_4365_ace4b9

Weiterführende Literatur

Empfehlungen zum selben Thema automatisch vorgeschlagen von bX