Barnes, A. D.; Charles, P. A.; Clark, J. S.; Cornelisse, R. and Knigge, C.
|DOI (Digital Object Identifier) Link:||http://doi.org/10.1063/1.2130278|
|Google Scholar:||Look up in Google Scholar|
Despite more than 20 years of study, we still possess only limited constraints on the fundamental properties of SS433. With the exception of the 13d period, orbital parameters are ill-constrained, and hence the nature of both compact object, a neutron star or black hole, or the mass donor are still unknown. However, newly acquired high resolution blue spectra, taken when the precessing disc is closest to edge-on, provide the strongest evidence yet for a massive, A4 supergiant donor, in addition to expanding the phase constraints for further observations of the donor.
|Item Type:||Journal Article|
|Academic Unit/Department:||Science > Physical Sciences
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Astrid Peterkin|
|Date Deposited:||17 Mar 2009 09:48|
|Last Modified:||15 Jan 2016 11:01|
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