Eric Agol , Stuart Wyithe, Barbara Jones, Omer Blaes, Chris Fluke, PASA, 18 (2), in press.
Next Section: Motivation
Mid-Infrared Imaging of the Einstein Cross QSO
Eric Agol 1,2
Stuart Wyithe3,4
Barbara Jones5
Omer Blaes6
Chris Fluke7
1 Chandra Fellow
2 Caltech, MS 130-33, Pasadena, CA, 91125, USA
agol@tapir.caltech.edu
3 School of Physics, University of Melbourne, Parkville, VIC 3052, Australia
swyithe@physics.unimelb.edu
4 Princeton University Observatory, Peyton Hall, Princeton, NJ 08544
5 Centre for Astrophysics and Space Sciences, University of California at San Diego, La Jolla, CA 92093, USA
b2jones@ucsd.edu
6 Physics Department, University of California, Santa Barbara, CA 93106, USA
blaes@gemini.physics.ucsb.edu
7 Center for Astrophysics and Supercomputing, Mail number 31, Swinburne University of Technology, PO Box 218, Hawthorn, VIC 3122, Australia
cfluke@swin.edu.au
Abstract:
Keywords: quasars: individual (Q2237+0305), gravitational lensing, radiation mechanisms: general, infrared: general
- Motivation
- Microlensing in the Einstein Cross
- Observations
- The Infrared Source is Due to Dust
- The IR Spectral Energy Distribution
- Conclusions
- References
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© Copyright Astronomical Society of Australia 1997