Luck, R. Earle; Heiter, Ulrike (2005). «Stars within 15 Parsecs: Abundances for a Northern Sample». The Astronomical Journal129 (2): 1063-1083. Bibcode:2005AJ....129.1063L. doi:10.1086/427250.
Luck, R. Earle; Heiter, Ulrike (2005). «Stars within 15 Parsecs: Abundances for a Northern Sample». The Astronomical Journal129 (2): 1063-1083. Bibcode:2005AJ....129.1063L. doi:10.1086/427250.
Siess, Lionel (2000). «Computation of Isochrones». Institut d'Astronomie et d'Astrophysique, Université libre de Bruxelles. Archivado desde el original el 10 de enero de 2014. Consultado el 6 de diciembre de 2007.—Compare, for example, the model isochrones generated for a ZAMS of 1.1 solar masses. This is listed in the table as 1.26 times the solar luminosity. At metallicity Z=0.01 the luminosity is 1.34 times solar luminosity. At metallicity Z=0.04 the luminosity is 0.89 times the solar luminosity.
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Siess, Lionel (2000). «Computation of Isochrones». Institut d'Astronomie et d'Astrophysique, Université libre de Bruxelles. Archivado desde el original el 10 de enero de 2014. Consultado el 6 de diciembre de 2007.—Compare, for example, the model isochrones generated for a ZAMS of 1.1 solar masses. This is listed in the table as 1.26 times the solar luminosity. At metallicity Z=0.01 the luminosity is 1.34 times solar luminosity. At metallicity Z=0.04 the luminosity is 0.89 times the solar luminosity.