Phase Resolved Blue Spectroscopy of SS433

Bibcode
2005AIPC..797..533B
DOI
10.1063/1.2130278
Barnes, A. D.; Charles, P. A.; Clark, J. S.; Cornelisse, R.; Knigge, C.
Referencia bibliográfica

INTERACTING BINARIES: Accretion, Evolution, and Outcomes. AIP Conference Proceedings, Volume 797, pp. 533-536 (2005).

Fecha de publicación:
10
2005
Número de autores
5
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
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.
Tipo
Sin árbitro
Estrellas binarias de rayos X
Espectroscopia

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