Chandra Observations of the Cloverleaf Quasar H1413+117: A Unique Laboratory for Microlensing Studies of a LoBAL Quasar
Abstract
We present new results uncovered by a reanalysis of a Chandra observation of the gravitationally lensed, low-ionization broad absorption line (LoBAL) quasar H1413+117. Previous analyses of the same Chandra observation led to the detection of a strong, redshifted Fe Kα line from the combined spectrum of all images. We show that the redshifted Fe Kα line is only significant in the brighter image A. The X-ray flux fraction of image A is larger by a factor of 1.55+/-0.17 than the optical R-band flux fraction, indicating that image A is significantly enhanced in the X-ray band. We also find that the Fe Kα line and the continuum are enhanced by different factors. A microlensing event could explain both the energy-dependent magnification and the significant detection of Fe Kα line emission in the spectrum of image A only. In the context of this interpretation, we provide constraints on the spatial extent of the inferred scattered continuum and reprocessed Fe Kα line emission regions in a LoBAL quasar.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- May 2004
- DOI:
- 10.1086/382743
- arXiv:
- arXiv:astro-ph/0401240
- Bibcode:
- 2004ApJ...606...78C
- Keywords:
-
- Cosmology: Gravitational Lensing;
- Galaxies: Quasars: Individual: Alphanumeric: H1413+117;
- X-Rays: Galaxies;
- Astrophysics
- E-Print:
- 12 pages, includes 4 figures, Accepted for publication in ApJ