WFPC2 Observations of NGC 454: an Interacting Pair of Galaxies
arXiv:astro-ph/9711058 · doi:10.1086/311115
Abstract
We present WFPC2 images in the F450W, F606W and F814W filters of the interacting pair of galaxies NGC 454. Our data indicate that the system is in the early stages of interaction. A population of young star-clusters has formed around the late component, and substantial amounts of gas have sunk into the center of the earlier component, where it has not yet produced significant visible star formation or nuclear activity. We have photometric evidence that the star-clusters have strong line emission, which indicate the presence of a substantial component of hot, massive stars which formed less than 5-10 Myrs ago.
14 pages, 4 figures, Latex (AAS macros), ApJL in press
References in corpus (1)
Cited by in corpus (8)
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- Advanced Camera for Surveys Observations of Young Star Clusters in the Interacting Galaxy UGC 10214
- NGC454: unveiling a new "changing look" AGN
- The NGC 454 system: anatomy of a mixed on-going merger
- Extended hard X-ray emission in highly obscured AGN
- Polarimetric imaging of interacting pairs