Discovery of a double peaked Fe emission line in the Cloverleaf quasar H1413+117

G. Chartas, Michael Eracleous, X. Dai, E. Agol, S. C. Gallagher

Research output: Contribution to journalArticle

1 Scopus citations

Abstract

Our spatial and spectral analysis of a recent deep Chandra observation of H 1413+117 confirms a microlensing event in a previous Chandra observation of this object performed about 5 years earlier. We present constraints on the structure of H 1413+117 based on the time-scale of this microlensing event. The analysis of the combined spectrum of the images indicates the presence of two emission line peaks at rest-frame energies of 5.35 keV and 6.32 keV and detected at the ≳ 97% and ≳ 99% confidence levels, respectively. The double peaked Fe emission is fit well with an accretion disk-line model, however, the best-fit accretion disk model parameters are neither well constrained nor unique. Another possible interpretation of the Fe emission is fluorescent Fe emission from the back-side of the wind. Additional observations are required to constrain better the model parameters.

Original languageEnglish (US)
Pages (from-to)1063-1066
Number of pages4
JournalAstronomische Nachrichten
Volume327
Issue number10
DOIs
StatePublished - Dec 1 2006

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'Discovery of a double peaked Fe emission line in the Cloverleaf quasar H1413+117'. Together they form a unique fingerprint.

  • Cite this