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Iron Spectra from Supermassive Black Holes:
Chandra Measures Iron in the Fire


Credit: X-ray spectra/NASA/CXC/MPI/M.Brusa et al.; Illustration: CXC/M.Weiss
JPEG (197.2 kb), Tiff (2.5 MB), PS (4.9 MB)

Using Chandra spectra obtained from more than 300 supermassive black holes in the centers of galaxies, a team of astronomers has been able to determine the amount of iron near the black holes (light blue in illustration on the right). The black holes were all located in the North and South Chandra Deep Fields, where the faintest and most-distant X-ray objects can be identified.

Click for large jpg
Chandra Deep Field-South
The left side of the above graphic shows portions of X-ray spectra from a subset of 50 black holes about 9 billion light years away (upper panel), and another group of 22 black holes that are about 11 billion light years away (lower panel). The peaks in the spectra are produced by X-ray emission from iron atoms, and indicate that approximately the same amount of iron was present around black holes 9 billion years and 11 billion years in the past.

Similar results corresponding to times ranging from 5 billion years to 9 billion years in the past show that the amount of iron around black holes has not changed significantly over the past 11 billion years. This implies that most of the iron in the galaxies that contain these supermassive black holes was created before the Universe was about 2 billion years old, when galaxies were very young.

Click for large jpg
Illustration of Fluorescence
The distinctive X-ray spectral peaks are produced by the fluorescence of iron atoms in a doughnut-shaped torus orbiting a supermassive black hole. In this process, high-energy X-rays from hot gas very near the black hole excite the iron atoms to a higher energy state, and they almost immediately return to their lower energy state with the emission of a lower-energy, fluorescent X-ray.

Fast Facts for Iron Spectra from Supermassive Black Holes:
Credit  X-ray spectra/NASA/CXC/MPI/M.Brusa et al.; Illustration: CXC/M.Weiss
Instrument  ACIS
References M. Brusa, R. Gilli, and A. Comastri, 2005. The Astrophysical Journal Letters, Volume 621, p. L5-L8; see also astro-ph/0501542
Release Date  May 23, 2005


Fast Facts for Chandra Deep Field-North:
Category  Cosmology/Deep Fields/X-ray Background, Black Holes
Coordinates (J2000)  RA 12h 36m 45.70s | Dec +62° 13' 58.00"
Constellation  Ursa Major
Observation Dates  20 pointings between Nov 13, 1999 & Feb 22, 2002
Observation Time  556 hours (23 days)
Obs. IDs  580, 967, 966, 957, 2386, 1671, 2344, 2232, 2233, 2423, 2234, 2421, 3293, 3388, 3408, 3389, 3409, 3294, 3390, 3391

Fast Facts for Chandra Deep Field-South :
Category  Cosmology/Deep Fields/X-ray Background, Black Holes
Coordinates (J2000)  RA 03h 32m 28s | Dec -27° 48' 30.00
Constellation  Fornax
Observation Dates  11 pointings between Oct 15, 1999 & Dec 23, 2000
Observation Time  278 hours (11.5 days)
Obs. IDs  1431_0, 1431_1, 441, 582, 2406, 2405, 2312, 1672, 2409, 2313, 2239

More Information on Iron Spectra from Supermassive Black Holes:
More Images of Iron Spectra from Supermassive Black Holes
Iron Spectra from Supermassive Black Holes Handout: html | pdf
Powerpoint and PDF
Related Chandra Images:
Photo Album: GOODS Chandra Deep Fields (19 Jun 03)
Photo Album: Lockman Hole (15 Feb 05)
Photo Album: GOODS Chandra Deep Field South (01 Jun 04)
More Information on Cosmology/Deep Fields/X-ray Background :
X-ray Astronomy Field Guide: Cosmology/Deep Fields/X-ray Background
Questions and Answers: Cosmology/Deep Fields/X-ray Background
Chandra Images: Cosmology/Deep Fields/X-ray Background
More Information on Black Holes:
X-ray Astronomy Field Guide: Black Holes
Questions and Answers: Black Holes
Chandra Images: Black Holes


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