Dust and gas in star-forming complexes in NGC 3351, NGC 5055, and NGC 5457
نویسندگان
چکیده
Abstract We present a study of the interstellar medium parameters in star-forming complexes (SFCs) NGC 3351, 5055, and 5457 galaxies. This concludes our previous investigations gas dust number spiral The data for three galaxies confirm following. There is tight correlation between near-infrared far-infrared luminosities extragalactic SFCs. Emission at 8 μm also shows strong with carbon monoxide emission. Atomic molecular masses do not show any corresponding velocity scatters; however, we see hint SFC largest scatter being located galaxy periphery.
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ژورنال
عنوان ژورنال: Baltic Astronomy
سال: 2023
ISSN: ['2543-6376']
DOI: https://doi.org/10.1515/astro-2022-0219