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Merge pull request #22 from eahussein/master
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resources/links/.ipynb_checkpoints/Angular resolution-checkpoint.md

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It seems that in astronomy, there is a relationship between the image resolution $\theta$ and the wavelength $\lambda$ giving by
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$$ \theta = 1.22 \frac{\lambda} {D} $$
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$\theta = 1.22 \frac{\lambda} {D}$
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- Where $D$ is the diameter of the telescope.
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- to get better resolution (small $\theta$), we need:

resources/links/Angular resolution.md

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**_SO THE GOAL BECOMES HOW TO MAKE IMAGES WITH SMALL ANGULAR RESOLUTIONS._**
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It seems that in astronomy, there is a relationship between the image resolution $\theta$ and the wavelength $\lambda$ giving by
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It seems that in astronomy, there is a relationship between the image resolution $\theta$ and the wavelength $\lambda$ giving by:
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$$\theta = 1.22 \frac{\lambda} {D}$$
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$$ \theta = 1.22 \frac{\lambda} {D} $$
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- Where $D$ is the diameter of the telescope.
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- to get better resolution (small $\theta$), we need:

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