Abstract
We have imaged the globular cluster NGC 7099 in the far-UV and visible with WFPC2 on the Hubble Space Telescope. Our far-UV images show a sparsely populated and fully resolved central region. The far-UV to visible color-magnitude diagram of these stars shows a well-defined horizontal branch with no evidence for hot, more evolved descendants. We find one hot horizontal branch star; the center of the cluster harbors four luminous blue stragglers. Far-UV images do not show any singularly steep density gradient at small radii among the horizontal branch stars of this post-core-collapse cluster.
Original language | English (US) |
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Pages (from-to) | 762-766 |
Number of pages | 5 |
Journal | Astrophysical Journal |
Volume | 461 |
Issue number | 2 PART I |
DOIs | |
State | Published - 1996 |
Externally published | Yes |
Keywords
- Globular clusters: individual (NGC 7099)
- Stars: evolution
- Stars: horizontal-branch
- Ultraviolet: stars
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science