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29 March 2024
 
  » arxiv » astro-ph/0009284

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Interstellar Gas and Star Formation Near the Peculiar Radio Galaxy NGC 4410A
Beverly J. Smith ; Megan Donahue ; John Stocke ;
Date 19 Sep 2000
Subject astro-ph
AffiliationEast Tennessee State University), Megan Donahue (Space Telescope Science Institute), and John Stocke (University of Colorado
AbstractWe 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.
Source arXiv, astro-ph/0009284
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