Richichi, A.; Roccatagliata, V. (2005). «Aldebaran's angular diameter: How well do we know it?». Astronomy & Astrophysics433 (1): 305–312. Bibcode:2005A&A...433..305R. arXiv:astro-ph/0502181. doi:10.1051/0004-6361:20041765. «We derive an average value of 19.96±0.03 milliarcsec for the uniform disk diameter. The corresponding limb-darkened value is 20.58±0.03 milliarcsec, or 44.2±0.9 R☉.»
Richichi, A.; Roccatagliata, V. (2005). «Aldebaran's angular diameter: How well do we know it?». Astronomy & Astrophysics433 (1): 305–312. Bibcode:2005A&A...433..305R. arXiv:astro-ph/0502181. doi:10.1051/0004-6361:20041765. «We derive an average value of 19.96±0.03 milliarcsec for the uniform disk diameter. The corresponding limb-darkened value is 20.58±0.03 milliarcsec, or 44.2±0.9 R☉.»
Koncewicz, R.; Jordan, C. (January 2007), «OI line emission in cool stars: calculations using partial redistribution», Monthly Notices of the Royal Astronomical Society374 (1): 220–231, Bibcode:2007MNRAS.374..220K, doi:10.1111/j.1365-2966.2006.11130.x
harvard.edu
adsabs.harvard.edu
Richichi, A.; Roccatagliata, V. (2005). «Aldebaran's angular diameter: How well do we know it?». Astronomy & Astrophysics433 (1): 305–312. Bibcode:2005A&A...433..305R. arXiv:astro-ph/0502181. doi:10.1051/0004-6361:20041765. «We derive an average value of 19.96±0.03 milliarcsec for the uniform disk diameter. The corresponding limb-darkened value is 20.58±0.03 milliarcsec, or 44.2±0.9 R☉.»
Koncewicz, R.; Jordan, C. (January 2007), «OI line emission in cool stars: calculations using partial redistribution», Monthly Notices of the Royal Astronomical Society374 (1): 220–231, Bibcode:2007MNRAS.374..220K, doi:10.1111/j.1365-2966.2006.11130.x
illinois.edu
stars.astro.illinois.edu
James B. Kaler (May 22, 2009). «Aldebaran». Stars. Arkivert frå originalen den 10. januar 2010. Henta 20. desember 2009.