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We investigate the distribution of gas (ionized, neutral atomic and molecular) and interstellar dust in the complex star‐forming region NGC 6357 with the goal of studying the interplay between the massive stars in the open cluster Pis 24 and the surrounding interstellar matter.
Our study of the distribution of the ionized gas is based on narrow‐band Hα, [S ii]and [O iii] images obtained with the Curtis–Schmidt...
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