巨蛇座NN (Chinese Wikipedia)

Analysis of information sources in references of the Wikipedia article "巨蛇座NN" in Chinese language version.

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aanda.org

存档副本. [2021-09-24]. （原始内容存档于2019-01-25）.

arxiv.org

Parsons; et al. Precise mass and radius values for the white dwarf and low mass M dwarf in the pre-cataclysmic binary NN Serpentis. 2009. arXiv:0909.4307 .
Chen. Can angular momentum loss cause the period change of NN Ser?. 2009. Bibcode:2009A&A...499L...1C. arXiv:0904.2319 . doi:10.1051/0004-6361/200911638.
Parsons; et al. Orbital Period Variations in Eclipsing Post Common Envelope Binaries. 2010. arXiv:1005.3958 .

doi.org

Chen. Can angular momentum loss cause the period change of NN Ser?. 2009. Bibcode:2009A&A...499L...1C. arXiv:0904.2319 . doi:10.1051/0004-6361/200911638.

exoplanet.eu

Schneider, J. Notes for star NN Ser. The Extrasolar Planets Encyclopaedia. [2010-10-22]. （原始内容存档于2010-10-15）.

harvard.edu

ui.adsabs.harvard.edu

Chen. Can angular momentum loss cause the period change of NN Ser?. 2009. Bibcode:2009A&A...499L...1C. arXiv:0904.2319 . doi:10.1051/0004-6361/200911638.

iop.org

Qian. A SUBSTELLAR COMPANION TO THE WHITE DWARF-RED DWARF ECLIPSING BINARY NN Ser. 2009.

web.archive.org

存档副本. [2021-09-24]. （原始内容存档于2019-01-25）.
Schneider, J. Notes for star NN Ser. The Extrasolar Planets Encyclopaedia. [2010-10-22]. （原始内容存档于2010-10-15）.