Interstellar Gas and Star Formation Near the Peculiar Radio Galaxy NGC 4410A

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dc.creatorSmith, Beverly J.
dc.creatorDonahue, Megan
dc.creatorStocke, John
dc.date2000-09-18
dc.date.accessioned2026-07-25T11:22:24Z
dc.descriptionWe present new multi-wavelength data for the NGC 4410 galaxy group. This group contains the peculiar radio galaxy NGC 4410A, which has a distorted double-lobed radio structure. NGC 4410A is strongly interacting with three nearby galaxies, and has a peculiar ring-like optical morphology, a number of luminous H II regions, as well as as tidal tails and bridges variously visible in optical, HI, and X-ray light. The gravitational interaction has affected the interstellar matter, the star formation rate, and the radio lobes in this system.
dc.descriptionProceedings of the Gas and Galaxy Evolution Conference. See also http://www.etsu.edu/physics/bsmith/research/n4410.html
dc.identifierhttps://arxiv.org/abs/astro-ph/0009284
dc.identifierhttp://arxiv.org/abs/astro-ph/0009284
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/2199
dc.subjectAstrophysics
dc.titleInterstellar Gas and Star Formation Near the Peculiar Radio Galaxy NGC 4410A
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