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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 | Affiliation: | East Tennessee State University), Megan Donahue (Space Telescope Science Institute), and John Stocke (University of Colorado | 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. | Source: | arXiv, astro-ph/0009284 | Services: | Forum | Review | PDF | Favorites |
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