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X-ray Imaging01:24

X-ray Imaging

German physicist Wilhelm Röntgen (1845–1923) was experimenting with electrical current when he discovered that a mysterious and invisible "ray" would pass through his flesh but leave an outline of his bones on a screen coated with a metal compound. In 1895, Röntgen made the first durable record of the internal parts of a living human: an "X-ray" image (as it came to be called) of his wife’s hand. Scientists worldwide quickly began their own experiments with X-rays, and by 1900, X-ray was widely...
Detection of Black Holes01:10

Detection of Black Holes

Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Schwarzschild Radius and Event Horizon01:21

Schwarzschild Radius and Event Horizon

No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape velocity with the...
Absorption of Radiation01:05

Absorption of Radiation

The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
The X̄ Chart00:58

The X̄ Chart

The  x̄ chart is a statistical tool for monitoring the means in a process.
The x̄ chart, often known as the individual control chart, is a crucial tool in statistical process control. It is designed to monitor process behavior and performance over time and is widely used in various industries to ensure that processes are operating at their optimum capacity and within specified limits.
A x̄ chart is constructed by plotting individual measurements of a quality characteristic in the order in which...
Imaging Studies for Cardiovascular System III: X-Ray01:20

Imaging Studies for Cardiovascular System III: X-Ray

The most common cardiovascular diagnostic test is an X-ray. It produces images of the heart, blood vessels, and adjacent structures.
Definition and Purpose
An X-ray, or radiograph, is a non-invasive method that uses ionizing radiation to take images of internal structures. It is mainly used in cardiac imaging to examine the heart, lungs, and major blood vessels, aiming to identify abnormalities in the heart's size, shape, and position, such as heart failure, congenital defects, and vascular...

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Related Experiment Video

Updated: Jun 15, 2026

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic
06:46

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic

Published on: August 25, 2016

X-raying galaxies: a Chandra legacy.

Q Daniel Wang1

  • 1Department of Astronomy, University of Massachusetts, Amherst, MA 01003, USA. wqd@astro.umass.edu

Proceedings of the National Academy of Sciences of the United States of America
|March 10, 2010
PubMed
Summary
This summary is machine-generated.

Chandra X-ray Observatory data reveals hot gas in nearby galaxies is concentrated locally, not in halos. This suggests most stellar feedback energy escapes galaxies via outflows, impacting galaxy evolution theories.

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Measurement of X-ray Beam Coherence along Multiple Directions Using 2-D Checkerboard Phase Grating
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Bringing the Visible Universe into Focus with Robo-AO
10:35

Bringing the Visible Universe into Focus with Robo-AO

Published on: February 12, 2013

Related Experiment Videos

Last Updated: Jun 15, 2026

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic
06:46

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic

Published on: August 25, 2016

Measurement of X-ray Beam Coherence along Multiple Directions Using 2-D Checkerboard Phase Grating
10:39

Measurement of X-ray Beam Coherence along Multiple Directions Using 2-D Checkerboard Phase Grating

Published on: October 11, 2016

Bringing the Visible Universe into Focus with Robo-AO
10:35

Bringing the Visible Universe into Focus with Robo-AO

Published on: February 12, 2013

Area of Science:

  • X-ray Astronomy
  • Galaxy Evolution
  • Astrophysics

Background:

  • Hot gas in and around galaxies is crucial for understanding galaxy formation and evolution.
  • Stellar and active galactic nuclear feedback processes are poorly understood drivers of this hot gas.

Purpose of the Study:

  • To review Chandra's contributions to understanding hot gas in nearby galaxies.
  • To characterize the properties and distribution of hot gas and its relation to feedback processes.

Main Methods:

  • Analysis of Chandra X-ray Observatory data.
  • Characterization of spatial, thermal, chemical, and kinetic properties of galactic hot gas.
  • Comparison of observations with galaxy formation and feedback simulations.

Main Results:

  • Hot gas in our galaxy is concentrated within a few kiloparsecs of the bulge and disk.
  • Chemically enriched hot gas on larger scales has low column density, likely not accounting for missing baryons.
  • X-ray emission correlates with star formation rate and stellar mass, indicating stellar feedback as the primary heating source.

Conclusions:

  • The bulk of stellar feedback energy and heavy elements likely escape galaxies through outflows.
  • Observed X-ray luminosity is a small fraction of feedback energy, supporting outflow models.
  • Understanding these outflows is key to comprehending galaxy evolution and circumgalactic medium interactions.