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- W2113125913 abstract "The region surrounding the active nucleus of the barred spiral galaxy NGC 1365 is observed in the (Oiii)5007 line and neighbouring continuum using the Faint Object Cam- era (FOC) aboard the Hubble Space Telescope (HST). In the continuum light numerous bright super star clusters (SSCs) are seen in the nuclear region. They tend to fall on an elongated ring around the nucleus and contribute about 20 % of the total continuumfluxinthiswavelengthregime.Withoutapplyingany extinction correction the brightest SSCs have an absolute lumi- nosity MB = 14: 1 0: 3 and are very compact with radii R < 3 pc. Complementary ground-based spectroscopy gives an extinction estimate AB =2 : m 5 0 : m 5 towards these regions, indicating a true luminosity MB = 16: 6 0: m 6. The bright compact radio source NGC 1365:A is found to coincide spatially with one of the SSCs. We conclude that it is a radio supernova. TheHSTobservationsresolvetheinnerstructureofthecon- ical outflow previously seen in the (Oiii)5007 line in ground- based observations, and reveal a complicated structure of in- dividual emission-line clouds, some of which gather in larger agglomerations. The total luminosity in the (Oiii) line amounts to L(OIII) ' 3:710 40 erg s 1 where about 40 % is emitted by the clouds." @default.
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- W2113125913 date "1997-12-01" @default.
- W2113125913 modified "2023-09-24" @default.
- W2113125913 title "IMAGING THE NUCLEAR ENVIRONMENT OF NGC 1365 WITH THE HUBBLE SPACE TELESCOPE" @default.
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