Barrado y Navascues, David; Stauffer, John R.; Hartmann, Lee; Balachandran, Suchitra C. (January 1997). “The Age of Gliese 879 and Fomalhaut”. Astrophysical Journal475: 313. arXiv:astro-ph/9704021. Bibcode: 1997ApJ...475..313B. doi:10.1086/303518. This paper lists [Fe/H] = -0.11 dex.
Kalas, Paul; Graham, James R.; Fitzgerald, Michael P.; Clampin, Mark (2013). “STIS Coronagraphic Imaging of Fomalhaut: Main Belt Structure and the Orbit of Fomalhaut b”. The Astrophysical Journal775 (1): article id. 56. arXiv:1305.2222. Bibcode: 2013ApJ...775...56K. doi:10.1088/0004-637X/775/1/56.
Di Folco, E.; Thévenin, F.; Kervella, P.; Domiciano de Souza, A.; Coudé du Foresto, V.; Ségransan, D.; Morel, P. (November 2004). “VLTI near-IR interferometric observations of Vega-like stars. Radius and age of α PsA, β Leo, β Pic, ɛ Eri and τ Cet”. Astronomy and Astrophysics426 (2): 601–617. Bibcode: 2004A&A...426..601D. doi:10.1051/0004-6361:20047189.This paper lists [Fe/H] = −0.10 dex.
Barrado y Navascues, David; Stauffer, John R.; Hartmann, Lee; Balachandran, Suchitra C. (January 1997). “The Age of Gliese 879 and Fomalhaut”. Astrophysical Journal475: 313. arXiv:astro-ph/9704021. Bibcode: 1997ApJ...475..313B. doi:10.1086/303518. This paper lists [Fe/H] = -0.11 dex.
The disc was reported by Holland, Wayne S. (1998). “Submillimetre images of dusty debris around nearby stars”. Nature392 (6678): 788–791. Bibcode: 1998Natur.392..788H. doi:10.1038/33874. They noted that the disc was centered on a cavity, which they suggested might have been swept out by planets.
Kalas, Paul; Graham, James R.; Fitzgerald, Michael P.; Clampin, Mark (2013). “STIS Coronagraphic Imaging of Fomalhaut: Main Belt Structure and the Orbit of Fomalhaut b”. The Astrophysical Journal775 (1): article id. 56. arXiv:1305.2222. Bibcode: 2013ApJ...775...56K. doi:10.1088/0004-637X/775/1/56.
Di Folco, E.; Thévenin, F.; Kervella, P.; Domiciano de Souza, A.; Coudé du Foresto, V.; Ségransan, D.; Morel, P. (November 2004). “VLTI near-IR interferometric observations of Vega-like stars. Radius and age of α PsA, β Leo, β Pic, ɛ Eri and τ Cet”. Astronomy and Astrophysics426 (2): 601–617. Bibcode: 2004A&A...426..601D. doi:10.1051/0004-6361:20047189.This paper lists [Fe/H] = −0.10 dex.
Johnson, H. L.; Iriarte, B.; Mitchell, R. I.; Wisniewskj, W. Z. (1966). “UBVRIJKL photometry of the bright stars”. Communications of the Lunar and Planetary Laboratory4 (99): 99. Bibcode: 1966CoLPL...4...99J.
Barrado y Navascues, David; Stauffer, John R.; Hartmann, Lee; Balachandran, Suchitra C. (January 1997). “The Age of Gliese 879 and Fomalhaut”. Astrophysical Journal475: 313. arXiv:astro-ph/9704021. Bibcode: 1997ApJ...475..313B. doi:10.1086/303518. This paper lists [Fe/H] = -0.11 dex.
The disc was reported by Holland, Wayne S. (1998). “Submillimetre images of dusty debris around nearby stars”. Nature392 (6678): 788–791. Bibcode: 1998Natur.392..788H. doi:10.1038/33874. They noted that the disc was centered on a cavity, which they suggested might have been swept out by planets.
Kalas, Paul; Graham, James R.; Fitzgerald, Michael P.; Clampin, Mark (2013). “STIS Coronagraphic Imaging of Fomalhaut: Main Belt Structure and the Orbit of Fomalhaut b”. The Astrophysical Journal775 (1): article id. 56. arXiv:1305.2222. Bibcode: 2013ApJ...775...56K. doi:10.1088/0004-637X/775/1/56.
ヨーロッパ・キリスト教勢力によって征服される直前のトレド(スペイン)で、アラビアの学者たちによって編纂された計算天文学の基本的書物。アラビア語原典は失われたが、ヨーロッパでラテン語訳が広く普及して残っているため、その内容を知ることができる。G. J. Toomer, "A Survey of the Toledan Tables". Osiris, vol, 15 (1968), pp. 5–174. アラビア語の原題は不明だが、アラビア語版のウィキペディアでは「アッ=ジージュ・アッ=トゥライトゥリー」 الزيج الطليطليaz-Zīǧ aṭ-Ṭulayṭulī / al-Zīj al-Ṭulayṭulī (“トレド・ジージュ”)と呼ばれている。
Paul Kalas (2008年11月13日). “Direct Image Of Extrasolar Planet”. 2016年11月6日閲覧。(at 3 minutes 45 seconds: "... has to be less than three Jupiter masses. In fact our lower limit to Fomalhaut b is Neptune")