Zusammenfassung
Using Hubble Space Telescope (HST) ACS/WFC data we present the photometry and
spatial distribution of resolved stellar populations in the outskirts of NGC
2915, a blue compact dwarf with an extended HI disc. These observations reveal
an elliptical distribution of red giant branch stars, and a clumpy distribution
of main-sequence stars that correlate with the HI gas distribution. We
constrain the upper-end initial mass function (IMF) and determine the star
formation law (SFL) in this field, using the observed main-sequence stars and
an assumed constant star formation rate. Previously published H\alpha
observations of the field, which show one faint HII region, are used to provide
further constraints on the IMF. We find that the main-sequence luminosity
function analysis alone results in a best-fitting IMF with a power-law slope
\alpha=-2.85 and upper-mass limit M$_u$ = 60 M$_ødot$. However, if we
assume that all H\alpha emission is confined to HII regions then the
upper-mass limit is restricted to M$_u$ $łe$20 M$_ødot$. For the
luminosity function fit to be correct we have to discount the H\alpha
observations implying significant diffuse ionized gas or escaping ionizing
photons. Combining the HST photometry with HI imaging we find the SFL has a
power law index $N=1.53 0.21$. Applying these results to the entire outer
HI disc indicates that it contributes 11--28% of the total recent star
formation in NGC 2915, depending on whether the IMF is constant within the disc
or varies from the centre to the outer region.
Nutzer