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

Beverly J. Smith·Megan Donahue·John Stocke
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Abstract

We 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.

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Beverly J. Smith, Megan Donahue, John Stocke. 2000-09-18. Interstellar Gas and Star Formation Near the Peculiar Radio Galaxy NGC 4410A. https://arxiv.org/abs/astro-ph/0009284

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