Celestial hemisphere:  Southern  ·  Constellation: Pavo (Pav)  ·  Contains:  IC 4820  ·  IC 4823  ·  NGC 6744
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NGC 6744 (Caldwell 101), Eduardo Rigoldi Fernandes
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NGC 6744 (Caldwell 101)

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NGC 6744 (Caldwell 101), Eduardo Rigoldi Fernandes
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NGC 6744 (Caldwell 101)

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Description

The spiral galaxy NGC 6744, also known as Caldwell 101, located in the constellation Pavo. Situated approximately 30 million light-years from Earth, NGC 6744 is one of the spiral galaxies most similar to our own Milky Way in terms of structure and dimensions.

NGC 6744 features a yellowish central nucleus, predominantly composed of older, metal-poor stars. Surrounding this nucleus, we can observe its vast spiral arms, filled with star-forming regions and emission nebulae, which appear in shades of blue and pink due to the intense activity of young, massive stars. This galaxy spans about 175,000 light-years, making it one of the largest known spiral galaxies.

It is interesting to note the small satellite galaxy visible in the image, which resembles the Large Magellanic Cloud, one of the Milky Way's satellites. This dwarf galaxy interacts gravitationally with NGC 6744, contributing to the dynamics and formation of new stars in the main galaxy's spiral arms.

Studying NGC 6744 provides valuable insights into the structure and evolution of spiral galaxies like our own. The observable features of NGC 6744, such as active star formation and the presence of satellite galaxies, allow astronomers to compare theoretical models with practical observations, deepening the understanding of galactic interactions and structure formation in the universe.

I used the clear filter as luminance for the RGB and subtracted the R from Ha.

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NGC 6744 (Caldwell 101), Eduardo Rigoldi Fernandes