QS Telescopii is a faint, well-studied[4]binary star system in the southern constellationTelescopium.[7] It is composed of a white dwarf and main sequencedonor star, locked into a close, circular orbit facing one another. Known as polars, material from the donor star does not form an accretion disk around the white dwarf, but rather streams directly onto it.[6] This is due to the presence of the white dwarf's strong magnetic field. The pair undergo frequent shifts between a high and low accretion states, and it shifts between single and double accretion poles. The main pole is partially self-eclipsing.[4]
^ abcdGerke, Jill R.; et al. (2006). "Polars Changing State: Multiwavelength Long-Term Photometry and Spectroscopy of QS Telescopii, V834 Centauri, and BL Hydri". Publications of the Astronomical Society of the Pacific. 118 (843): 678–86. arXiv:astro-ph/0603097. Bibcode:2006PASP..118..678G. doi:10.1086/503753. S2CID14857705.
Romero-Colmenero, E.; et al. (August 2005). Hameury, J.-M.; Lasota, J.-P. (eds.). An eclipsing geometry for the polar QS Tel. The Astrophysics of Cataclysmic Variables and Related Objects, Proceedings of ASP Conference. Vol. 330. San Francisco: Astronomical Society of the Pacific. p. 429. Bibcode:2005ASPC..330..429R.
de Martino, D.; et al. (January 1998). "Insights into the accretion flow in QS Telescopii (RE1938-461) from HST observations". Astronomy and Astrophysics. 329: 571–578. Bibcode:1998A&A...329..571D.
Clayton, K. L.; et al. (1996). Evans, A.; Wood, Janet H. (eds.). Recent progress on the polar QS Tel: the HST results. Cataclysmic variables and related objects. Proceedings of the 158th colloquium of the International Astronomical Union (IAU); held at Keele; United Kingdom; June 26-30; 1995; Dordrecht. Astrophysics and Space Science Library. Kluwer Academic Publishers. p. 225. Bibcode:1996ASSL..208..225C. doi:10.1007/978-94-009-0325-8_68.
de Martino, D.; Buckely, D. A. H.; Mouchet, M.; Mukai, K. (June 1995). "UV observations of the polar system RE 1938-461". Astronomy and Astrophysics. 298: L5. Bibcode:1995A&A...298L...5D.
Rosen, S.; et al. (1995). Buckley, D. A. H.; Warner, B. (eds.). EUVE Spectrophotometry of QS Tel (RE1938-461): The Second Pole Becomes Active. Cape Workshop on Magnetic cataclysmic variables; Proceedings of the Cape Workshop, held in Cape Town, 23-27 January 1995. Astronomical Society of the Pacific Conference Series. Vol. 85. San Francisco: Astronomical Society of the Pacific. p. 279. Bibcode:1995ASPC...85..279R.
Schwope, A. D.; et al. (January 1995). "Two-pole accretion in the high-field polar RXJ 1938.6-4612". Astronomy and Astrophysics. 293: 764–776. Bibcode:1995A&A...293..764S.
Warren, John K.; et al. (September 1993). "Extreme Ultraviolet Explorer Observations of the Magnetic Cataclysmic Variable RE 1938-461". Astrophysical Journal Letters. 414: L69. Bibcode:1993ApJ...414L..69W. doi:10.1086/186998.
Warren, J. K.; et al. (December 1992). EUVE Observations of the Magnetic Cataclysmic Variable RE1938-461. American Astronomical Society, 181st AAS Meeting. Bulletin of the American Astronomical Society. Vol. 24. p. 1250. Bibcode:1992AAS...181.8007W. 80.07.