HST spectrum and timing of the ultracompact X-ray binary candidate 47 Tuc X9
To confirm the nature of the donor star in the ultracompact X-ray binary candidate 47 Tuc X9, we obtained optical spectra (3000–10 000 Å) with the Hubble Space Telescope / Space Telescope Imaging Spectrograph. We find no strong emission or absorption features in the spectrum of X9. In particular, we...
| Main Authors: | Tudor, V., Miller-Jones, James, Knigge, C., Maccarone, T., Tauris, T., Bahramian, A., Chomiuk, L., Heinke, C., Sivakoff, G., Strader, J., Plotkin, R., Soria, R., Albrow, M., Anderson, G., van den Berg, M., Bernardini, F., Bogdanov, S., Britt, C., Russell, D., Zurek, D. |
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| Format: | Journal Article |
| Published: |
Oxford University Press
2018
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| Online Access: | http://purl.org/au-research/grants/arc/FT140101082 http://hdl.handle.net/20.500.11937/69141 |
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