Epsilon Eridani (Malay Wikipedia)

Analysis of information sources in references of the Wikipedia article "Epsilon Eridani" in Malay language version.

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arxiv.org

books.google.com

  • From Epsilon Eridani, the Sun would appear on the diametrically opposite side of the sky at the coordinates RA=15j 32m 55.84496s, Dec=09° 27′ 29.7312″, which is located near Alpha Serpentis. The absolute magnitude of the Sun is 4.83,[a] so, at a distance of 3.212 parsecs, the Sun would have an apparent magnitude: ,[b] assuming negligible extinction (AV) for a nearby star.
    Ref.:
    1. Binney, James; Merrifield, Michael (1998), Galactic Astronomy, Princeton University Press, m/s. 56, ISBN 0691025657
    2. Gill, David; Elkin, W. L. (1884), Heliometer determinations of stellar parallaxes in the southern hemisphere, London, U.K.: The Royal Astronomical Society, m/s. 174–180.
    3. Gill, David (1893), Heliometer observations for determination of stellar parallax, London: Eyre and Spottiswoode, m/s. xvi.

caltech.edu

irsa.ipac.caltech.edu

doi.org

exoplanet.eu

gsu.edu

astro.gsu.edu

harvard.edu

ui.adsabs.harvard.edu

cfa.harvard.edu

msu.su

sai.msu.su

u-strasbg.fr

vizier.u-strasbg.fr

simbad.u-strasbg.fr

wikipedia.org

en.wikipedia.org

  • Evans, D. S. (June 20–24, 1966), "The revision of the general catalogue of radial velocities", Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30, University of Toronto: International Astronomical Union, 30, m/s. 57, Bibcode:1967IAUS...30...57E. Unknown parameter |editors= ignored (bantuan)
  • Buccino, A. P.; Mauas, P. J. D.; Lemarchand, G. A. (June 2003), "UV Radiation in Different Stellar Systems", Bioastronomy 2002: Life Among the Stars, Proceedings of IAU Symposium #213, San Francisco: Astronomical Society of the Pacific, 213, m/s. 97, Bibcode:2004IAUS..213...97B. Unknown parameter |editors= ignored (bantuan)