How are X-rays used in astrophysics and astronomy?
Very hot objects with very high temperature million degree K emit X- rays.
Stars with high temperature, matter falling into event horizon of black hole, etc emit radiation in X ray wave length. Since our atmosphere is not transparent to X rays, we have to send X ray telescopes to space or in balloons to high altitude.
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At night we see many stars, if there's a clear sky
Mostly we see them as tiny, white objects in sky .
The stars are not really so white , some are lot more red and some are blue , The thing that used to surprise me a lot was that blue stars are much hotter than the red ones .
What about X-rays , the are light waves of frequency more than ultraviolet and less than gamma rays , the are not a part of visible spectrum .
But what about their use ?
some stars do emit x-rays , showing their extremely high temperature .
satellites with x-ray detectors are used to detect such stars .
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X-rays are used in astrophysics and astronomy to study high-energy phenomena such as black holes, neutron stars, supernovae remnants, and active galactic nuclei. X-ray telescopes, such as Chandra X-ray Observatory and XMM-Newton, detect and analyze X-rays emitted by celestial objects. These observations provide insights into the behavior, composition, and dynamics of celestial bodies and phenomena that cannot be observed using other wavelengths of light.
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When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
- What is interferometric coherence?
- What type of radiation is the electromagnetic spectrum?
- Does the Milky Way have an active galactic nucleus? Is it or is it a type 1 or type 2 Seyfert galaxy?
- If x-rays are normally absorbed by the earth's atmosphere, how do astronomers overcome this issue when studying celestial temperatures?
- What is polarization? How is it related to the study of astronomy?
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