A Multiwavelength View of the Neutron Star Binary 1FGL J1417.7-4402: A Progenitor to Canonical Millisecond Pulsars
The Fermi γ-ray source 1FGL J1417.7–4407 (J1417) is a compact X-ray binary with a neutron star primary and a red giant companion in a ~5.4 days orbit. This initial conclusion, based on optical and X-ray data, was confirmed when a 2.66 ms radio pulsar was found at the same location (and with the same...
| Main Authors: | Swihart, S., Strader, J., Shishkovsky, L., Chomiuk, L., Bahramian, A., Heinke, C., Miller-Jones, James, Edwards, P., Cheung, C. |
|---|---|
| Format: | Journal Article |
| Published: |
Institute of Physics Publishing
2018
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| Online Access: | http://purl.org/au-research/grants/arc/FT140101082 http://hdl.handle.net/20.500.11937/71805 |
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