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27 April 2024
 
  » arxiv » astro-ph/0011208

 Article overview



The Discovery of a Giant H-alpha Filament in NGC 7213
Salman Hameed ; David Blank ; Lisa Young ; Nick Devereux ;
Date 10 Nov 2000
Subject astro-ph
AffiliationNMSU), David Blank (U. Sydney, ATNF), Lisa Young (NM-Tech), and Nick Devereux (Embry-Riddle
AbstractThe nearby Seyfert galaxy NGC 7213 has been imaged in H-alpha and HI with the CTIO 1.5 m telescope and with the Australia Telescope Compact Array (ATCA), respectively. Optically NGC 7213 looks undisturbed and relatively featureless but the continuum-subtracted H-alpha image shows a 19 kpc long filament located approximately 18.6 kpc from the nucleus. The H-alpha filament could be neutral gas photo-ionized by the active nucleus, as has been suggested for the Seyfert galaxy NGC 5252, or shock-ionized by a jet interacting with the surrounding HI, as has been suggested for the radio galaxy PKS 2240-41. The HI map reveals NGC 7213 to be a highly disturbed system suggesting a past merging event.
Source arXiv, astro-ph/0011208
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