Hα regions in FCC046 and FCC207

Autor(en)
D. Michielsen, S. De Rijcke, H. Dejonghe, W. W. Zeilinger, G. K.T. Hau
Abstrakt

We present deep Hα+[NII] narrowband imaging of FCC046 and FCC207, two dwarf ellipticals (dEs) in the Fornax Cluster. Although one does not expect much of an interstellar medium (ISM) to be present in dEs, FCC207 shows a central emission region, whereas FCC046 also contains fainter emission regions. The central emission can be explained as photo-ionization by post-AGB stars. Some of the emission clouds in FCC046 are resolved and have diameters of the order of 50-150 pc and Hα luminosities of 1030 W, comparable to supernova remnants (SNRs), pointing to recent star formation. Dwarfs like FCC046 could be the evolutionary link between normal, quiescent dEs and more vigorously starforming blue compact dwarfs (BCDs).

Organisation(en)
Institut für Astrophysik
Externe Organisation(en)
Ghent University , European Southern Observatory (Germany)
Journal
Astrophysics and Space Science
Band
284
Seiten
635-638
Anzahl der Seiten
4
ISSN
0004-640X
DOI
https://doi.org/10.1023/A:1024030711455
Publikationsdatum
2003
Peer-reviewed
Ja
ÖFOS 2012
103003 Astronomie, 103004 Astrophysik
Schlagwörter
ASJC Scopus Sachgebiete
Astronomy and Astrophysics, Space and Planetary Science
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/43fdc34b-15e0-4892-92cd-b0ead61befbc