Biermann, Peter L.; Falcke, Heino (1998). «Frontiers of Astrophysics: Workshop Summary». En Panvini, Robert S.; Weiler, Thomas J., eds. Fundamental particles and interactions: Frontiers in contemporary physics an international lecture and workshop series. AIP Conference Proceedings423. American Institute of Physics. pp. 236-248. Bibcode:1998AIPC..423..236B. ISBN1-56396-725-1. arXiv:astro-ph/9711066. doi:10.1063/1.55085.
astronomia.net
Pedro J. Hernández (2003). «La nueva cosmología». Consultado el 5 de febrero de 2008.
Case, Stephen (2015), «'Land-marks of the universe': John Herschel against the background of positional astronomy», Annals of Science72 (4): 417-434, Bibcode:2015AnSci..72..417C, PMID26221834, doi:10.1080/00033790.2015.1034588, «The great majority of astronomers working in the early nineteenth century were not interested in stars as physical objects. Far from being bodies with physical properties to be investigated, the stars were seen as markers measured in order to construct an accurate, detailed and precise background against which solar, lunar and planetary motions could be charted, primarily for terrestrial applications.».
McCracken, Garry; Stott, Peter (1 de enero de 2013). McCracken, Garry; Stott, Peter, eds. Fusion(en inglés) (Second edición). Boston: Academic Press. p. 13. ISBN978-0-12-384656-3. doi:10.1016/b978-0-12-384656-3.00002-7. «Eddington had realized that there would be a mass loss if four hydrogen atoms combined to form a single helium atom. Einstein’s equivalence of mass and energy led directly to the suggestion that this could be the long-sought process that produces the energy in the stars! It was an inspired guess, all the more remarkable because the structure of the nucleus and the mechanisms of these reactions were not fully understood.»
Biermann, Peter L.; Falcke, Heino (1998). «Frontiers of Astrophysics: Workshop Summary». En Panvini, Robert S.; Weiler, Thomas J., eds. Fundamental particles and interactions: Frontiers in contemporary physics an international lecture and workshop series. AIP Conference Proceedings423. American Institute of Physics. pp. 236-248. Bibcode:1998AIPC..423..236B. ISBN1-56396-725-1. arXiv:astro-ph/9711066. doi:10.1063/1.55085.
Case, Stephen (2015), «'Land-marks of the universe': John Herschel against the background of positional astronomy», Annals of Science72 (4): 417-434, Bibcode:2015AnSci..72..417C, PMID26221834, doi:10.1080/00033790.2015.1034588, «The great majority of astronomers working in the early nineteenth century were not interested in stars as physical objects. Far from being bodies with physical properties to be investigated, the stars were seen as markers measured in order to construct an accurate, detailed and precise background against which solar, lunar and planetary motions could be charted, primarily for terrestrial applications.».
Payne, C. H. (1925), Stellar Atmospheres; A Contribution to the Observational Study of High Temperature in the Reversing Layers of Stars (PhD Thesis), Cambridge, Massachusetts: Radcliffe College, Bibcode:1925PhDT.........1P.
Biermann, Peter L.; Falcke, Heino (1998). «Frontiers of Astrophysics: Workshop Summary». En Panvini, Robert S.; Weiler, Thomas J., eds. Fundamental particles and interactions: Frontiers in contemporary physics an international lecture and workshop series. AIP Conference Proceedings423. American Institute of Physics. pp. 236-248. Bibcode:1998AIPC..423..236B. ISBN1-56396-725-1. arXiv:astro-ph/9711066. doi:10.1063/1.55085.
Case, Stephen (2015), «'Land-marks of the universe': John Herschel against the background of positional astronomy», Annals of Science72 (4): 417-434, Bibcode:2015AnSci..72..417C, PMID26221834, doi:10.1080/00033790.2015.1034588, «The great majority of astronomers working in the early nineteenth century were not interested in stars as physical objects. Far from being bodies with physical properties to be investigated, the stars were seen as markers measured in order to construct an accurate, detailed and precise background against which solar, lunar and planetary motions could be charted, primarily for terrestrial applications.».
McCracken, Garry; Stott, Peter (1 de enero de 2013). McCracken, Garry; Stott, Peter, eds. Fusion(en inglés) (Second edición). Boston: Academic Press. p. 13. ISBN978-0-12-384656-3. doi:10.1016/b978-0-12-384656-3.00002-7. «Eddington had realized that there would be a mass loss if four hydrogen atoms combined to form a single helium atom. Einstein’s equivalence of mass and energy led directly to the suggestion that this could be the long-sought process that produces the energy in the stars! It was an inspired guess, all the more remarkable because the structure of the nucleus and the mechanisms of these reactions were not fully understood.»
