HR 1614 (Korean Wikipedia)

Analysis of information sources in references of the Wikipedia article "HR 1614" in Korean language version.

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aanda.org

S. Feltzing, G. Gonzalez (2001). “The nature of super-metal-rich stars. Detailed abundance analysis of 8 super-metal-rich star candidates”. 《Astronomy and Astrophysics》 367 (2): 253–265. doi:10.1051/0004-6361:20000477.

doi.org

dx.doi.org

S. Feltzing, G. Gonzalez (2001). “The nature of super-metal-rich stars. Detailed abundance analysis of 8 super-metal-rich star candidates”. 《Astronomy and Astrophysics》 367 (2): 253–265. doi:10.1051/0004-6361:20000477.
Eggen, O. J. (1992). “HR 1614 and the dissolution of a supercluster”. 《Astronomical Journal》 104 (5): 1906–1915. doi:10.1086/116366.

harvard.edu

adsabs.harvard.edu

Eggen, O. J. (1992). “HR 1614 and the dissolution of a supercluster”. 《Astronomical Journal》 104 (5): 1906–1915. doi:10.1086/116366.
S. Feltzing, J. Holmberg (2000). “The reality of old moving groups - the case of HR 1614. Age, metallicity, and a new extended sample”. 《Astronomy and Astrophysics》 357: 153–163.

mtwilson.edu

“H-K Project: Activity Cycles”. Mt. Wilson Observatory. 2007년 2월 9일에 원본 문서에서 보존된 문서. 2006년 12월 4일에 확인함.

u-strasbg.fr

simbad.u-strasbg.fr

“HD 32147 -- High proper-motion Star” (영어). Centre de Données astronomiques de Strasbourg. 2006년 6월 8일에 확인함.

web.archive.org

“H-K Project: Activity Cycles”. Mt. Wilson Observatory. 2007년 2월 9일에 원본 문서에서 보존된 문서. 2006년 12월 4일에 확인함.