Sign on

SAO/NASA ADS Astronomy Abstract Service


· Find Similar Abstracts (with default settings below)
· Full Refereed Journal Article (PDF/Postscript)
· Full Refereed Scanned Article (GIF)
· References in the article
· Citations to the Article (147) (Citation History)
· Refereed Citations to the Article
· SIMBAD Objects (1)
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
Optical caustics in a kerr spacetime and the origin of rapid X-ray variability in active galactic nuclei
Authors:
Rauch, Kevin P.; Blandford, Roger D.
Affiliation:
AA(California Institute of Technology, Pasadena, CA, US), AB(California Institute of Technology, Pasadena, CA, US)
Publication:
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 421, no. 1, p. 46-68 (ApJ Homepage)
Publication Date:
01/1994
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
Accretion Disks, Active Galactic Nuclei, Black Holes (Astronomy), Caustics (Optics), X Rays, Astrophysics, Light Curve, Ray Tracing, Variations
DOI:
10.1086/173625
Bibliographic Code:
1994ApJ...421...46R

Abstract

A detailed analysis of the optical caustic structure around rotating black holes is given, including a discussion of their possible relevance to rapid X-ray variability in active galactic nuclei (AGNs). It is found that the primary caustic surface takes the form of a small tube with an astroid (four-cusped) cross section. At large distances behind the hole, the tube is oriented parallel to the optic axis, but displaced transversely from it by a distance stet sin theta0 where stet is the spin of the hole in geometrical units and theta0 is the inclination angle of the distant observer from the pole. The transverse size s and central magnification M0 of the caustic are found to vary asymptotically as s approximately 0.34a2 sin2 theta0 r-1 and M0 approximately (22M1/2/(a2 sin2 theta0)) r3/2 (where M is the hole mass), respectively, in agreement with the results of an analytic, asymptotic analysis performed for theta0 = pi/2. The magnification is surprisingly high everywhere within the caustic. A fast, efficient, general-purpose code to trace geodesics in a Kerr metric is described, the calculation of the caustic structure of the Kerr metric representing an initial application. Sample light curves for point sources on geodesic orbits crossing the caustic are computed; in general, the lensing dominates all other features. The influence of caustics in computing the appearance of thick accretion disk models is examined. The importance of caustics in real AGNs depends on the geometry of the emitting matter; they could be important for disks and especially for jets, in which a significant fraction of the emitting material can reside near a caustic, for suitably oriented observers.

Printing Options

Print whole paper
Print Page(s) through

Return 600 dpi PDF to Acrobat/Browser. Different resolutions (200 or 600 dpi), formats (Postscript, PDF, etc), page sizes (US Letter, European A4, etc), and compression (gzip,compress,none) can be set through the Printing Preferences



More Article Retrieval Options

HELP for Article Retrieval


Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)


Find Similar Abstracts:

Use: Authors
Title
Keywords (in text query field)
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints