Exploring the Universe at X-rays - IUCAA-RPLiucaa-rpl.weebly.com/.../gulab_xrays.compressed.pdf ·...
Transcript of Exploring the Universe at X-rays - IUCAA-RPLiucaa-rpl.weebly.com/.../gulab_xrays.compressed.pdf ·...
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Exploring the Universe at X-rays
Gulab Chand DewanganIUCAA, Pune
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What are X-rays?What are their properties?
How are X-rays produced ?
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Discovery of X-rays
Discovered by Rontgen quite by an accident when experimenting with vacuum tubes.
High Voltage applied to the Electrodes produced faint glow on a fluorescent screen.
The faint glow was caused by unknown radiation - X-rays.
W. C. Rontgen
(8 November 1895)
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Properties of X-rays
Rontgen found that X-rays pass through
lighter elements (paper, wood, aluminum)
Stopped by heavy elements such as gold.
X-rays are electromagnetic radiation, like light but with much higher energy.
Mrs. Röntgen's hand - first X-ray picture of the human body.
C (Z=6), O (Z=8) in the flesh, Ca (Z=20) in the bones,Gold (Z=79) in the ring
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VisibleUV -ray
Radio MicrowaveIR
X-ray
Different types of radiation
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How are X-rays generated?
X-ray photons are nearly 1000 times more energetic than optical photons
Produced in Hot plasma (more than million degree K)
High energy particles
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X-ray Producing Collision Atomic Emission
Inverse Compton Scattering Synchrotron Radiation
How X-rays are generated?
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What is X-ray astronomy ?
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• Sun
• X-ray binaries
• Supernova
• Active Galaxies
• Galaxy Clusters
etc.
X-ray astronomy is the study of X-rays that come from natural sources in the Universe.
Sources like:
NGC 4697: X-ray sources in Elliptical Galaxy
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X-ray Astronomy Vs Medical X-rays
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Where are all the X-ray observatories?
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X-rays are high in energy but have short wavelengths.
Also, due to their short wavelengths they pass right through traditional mirrors used to focus visible light.
X-rays from space are absorbed by oxygen and nitrogen molecules in the Earth’s atmosphere.
These detectors are placed above the Earth’s atmosphere.
Astronomers must build special detectors to observe X-rays.
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Xe
Atom of XenonX-ray photoncoming fromhot body
X-ray detection in a Proportional Counter
e- An electron is dislodged
The free electron is accelerated by the detector electric field, bumping out even more electrons in other Xenon atoms along its route to the anode wire. This process happens over and over again for EACH photon that hits the Xe gas!!
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How did X-ray astronomy begin?
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Our Sun as an X-ray Source
September 1949: first detection of X-rays from Sun using captured German rockets from WW-II.
Weak X-ray emission – about one millionth of its total energy radiated
X-rays from solar corona – hot outer layers of sun's atmosphere.
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X-rays from Stars
People thought that X-rays from distant stars not possible to detect.
In 1950s & 60s, many thought NO X-ray astronomy!
Breakthrough experiment in 1962 by Bruno Rossi, Riccardo Giacconi, and collaborators at AS&E in Cambridge, MA.
After two failures of the Aerobee rocket, they successfully launched a detector to look for X-ray emission from the moon.
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The first extra-solar X-ray detection
Scorpius X-1.
Further rocket experiments in the 1960s found many other X-ray sources.
- and thus X-ray astronomy born!
Giacconi et al., 1962
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X-rays bouncing off of the mirrors and converging at one specific spot (the focus).
Advanced Technology – X-ray mirrors & solid state detectors
The shape is round and it is made up of individual sections of mirrors.
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Chandra X-ray Satellite -ray passing
High Resolution X-ray Images
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Riccardo Giacconi receives 2002 Physics Nobel Prize from King of Sweden
Nobel Prize in X-ray astronomy
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Rossi X-ray Timing Explorer(XTE, launched 1995)
Chandra (launched 1999)
XMM-Newton(launched 1999)
All X-ray observatories are on satellites
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What are the various types of X-ray sources in the Universe?
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X-rays from Stars
Young stars in the Orion nebula
Pre-Main Sequence Stars - X-ray emission from solar like magnetic activitiy
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Planetary nebula Expanding glowing shell of ionized gas ejected during the red giant phase of sun-like stars
Speed of the filaments ~ 6 million km/hour
HST + Chandra
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Supernova & Remnants - End stages of massive stars
Artist’s animation + Cas A observed Chandra
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2000 yrs old supernova remnant and the central neutron star
RCW 103
10000 ly away
One rotation in 5.7 hours
Too slow for a NS of this age
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Pulsars & pulsar wind Nebula(Crab nebula & pulsar)
Crab pulsar
ChandraHSTSpitzer
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The Crab Pulsar & Nebula
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Neutron star in a binary -An Artist’s View
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Black Holes & Neutron stars
Nuclear reactionsEfficiency ~ 0.7%
Accretion of matterOnto a neutron starEfficiency ~ 10%
Sco X-1 is powered by accretion on to a neutron star.
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Black Hole X-ray Binary
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Galaxies Massive, gravitationally bound
systems with multiple components – stars, gas, dust, black holes, NS, etc.
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Active Galaxies -Very bright nucleus
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Active Galactic Nuclei
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Active Galactic Nuclei
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Active Galactic Nuclei -Effects of BH on X-ray emission
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Active Galactic Nuclei -Spinning and Non-Spinning BHs
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Clusters of galaxies - Largest bound systems
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Clusters of galaxies - Radio jets/lobes in the X-ray cavity
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The distant universe Chandra Deep Field
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Rapid Progress ….
In the last 50 years, X-ray Astronomy has progressed so much that optical astronomy took four hundred years.
Detailed X-ray nature of nearby sources.
X-ray emission from the farthest of the universe.
Probing the most energetic phenomena in the universe.
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Indian X-ray Astronomy ASTROSAT - Indian X-ray/UV astronomy Satellite
UVIT
To be launched in 2013
4 X-ray & one UV/Optical instrument
Simultaneous multi- wavelengths observations
All sky X-ray monitor for Transients
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Thank You