Abstract
We have imaged the nucleus of M32 at 1600 Å (FUV) and 5500 Å (V) using the Wide-Field/Planetary Camera 2 (WFPC2) aboard the Hubble Space Telescope. We detected the nucleus at 1600 A using the redleak-free Woods filter on WFPC2. The far-ultraviolet (FUV) light profile can be fitted with a Gaussian of FWHM 0″.46 (4.6 pixels) but cannot be resolved into individual stars; no UV-bright nuclear structure was detected. The (FUV -V) color of the nucleus is 4.9 ± 0.3, which is consistent with earlier observations. We are unable to confirm any radial variation in (FUV -V) within 0″.8 of the nucleus; beyond that radius the FUV surface brightness drops below our detection threshold. We also performed surface photometry in V and found our results to be in excellent agreement with deconvolved WFPC1 results. M32's light profile continues to rise in a nuclear cusp even within 0″.1 of its center. No intermediate-age stellar population is required by evolutionary population synthesis models to reproduce the (FUV -V) color of the nucleus, although these data and current models are insufficient to resolve this issue.
Original language | English (US) |
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Pages (from-to) | 230-235 |
Number of pages | 6 |
Journal | Astrophysical Journal |
Volume | 505 |
Issue number | 1 PART I |
DOIs | |
State | Published - 1998 |
Externally published | Yes |
Keywords
- Galaxies: individual (M32)
- Galaxies: nuclei
- Galaxies: stellar content ultraviolet: galaxies
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science