Röntgenbinär (Swedish Wikipedia)

Analysis of information sources in references of the Wikipedia article "Röntgenbinär" in Swedish language version.

refsWebsite

Global rank Swedish rank

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low place

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arxiv.org

Liu, Q. Z; Van Paradijs, J; Van Den Heuvel, E. P. J. ”A catalogue of low-mass X-ray binaries in the Galaxy, LMC, and SMC (Fourth edition)” (på engelska). Astronomy and Astrophysics 469 (2): sid. 807. doi:10.1051/0004-6361:20077303. Läst 15 september 2019.
Tauris, Thomas M; Van Den Heuvel, Edward P. J; Savonije, Gerrit J. ”Formation of Millisecond Pulsars with Heavy White Dwarf Companions:Extreme Mass Transfer on Subthermal Timescales” (på engelska). The Astrophysical Journal 530 (2): sid. L93-L96. doi:10.1086/312496. PMID 10655173. Läst 15 september 2019.
Podsiadlowski, Ph; Rappaport, S; Pfahl, E. D (2002). ”Evolutionary Sequences for Low- and Intermediate-Mass X-Ray Binaries” (på engelska). The Astrophysical Journal 565 (2): sid. 1107. doi:10.1086/324686. Läst 15 september 2019.
Tauris, Thomas M; Van Den Heuvel, Edward P. J; Savonije, Gerrit J. ”Formation of Millisecond Pulsars with Heavy White Dwarf Companions:Extreme Mass Transfer on Subthermal Timescales” (på engelska). The Astrophysical Journal 530 (2): sid. L93-L96. doi:10.1086/312496. PMID 10655173. Läst 15 september 2019.

”GCVS Variability Types” (på engelska). General Catalogue of Variable Stars. Russian Foundation for Basic Research, Sternberg Astronomical Institute, Moskva, Ryssland. http://www.sai.msu.su/gcvs/gcvs/iii/vartype.txt. Läst 31 juli 2019.

Tauris, Thomas M; Van Den Heuvel, Edward P. J; Savonije, Gerrit J. ”Formation of Millisecond Pulsars with Heavy White Dwarf Companions:Extreme Mass Transfer on Subthermal Timescales” (på engelska). The Astrophysical Journal 530 (2): sid. L93-L96. doi:10.1086/312496. PMID 10655173. Läst 15 september 2019.
Tauris, Thomas M; Van Den Heuvel, Edward P. J; Savonije, Gerrit J. ”Formation of Millisecond Pulsars with Heavy White Dwarf Companions:Extreme Mass Transfer on Subthermal Timescales” (på engelska). The Astrophysical Journal 530 (2): sid. L93-L96. doi:10.1086/312496. PMID 10655173. Läst 15 september 2019.