Elektra (stjärna) (Swedish Wikipedia)

Analysis of information sources in references of the Wikipedia article "Elektra (stjärna)" in Swedish language version.

refsWebsite

Global rank Swedish rank

9doi.org

2^nd place

14^th place

4arxiv.org

69^th place

415^th place

1books.google.com

3^rd place

37^th place

1iau.org

1,985^th place

1,166^th place

1rochester.edu

2,691^st place

3,783^rd place

arxiv.org

Van Leeuwen, F. (2007). ”Validation of the new Hipparcos reduction”. Astronomy and Astrophysics 474 (2): sid. 653. doi:10.1051/0004-6361:20078357. https://arxiv.org/abs/0708.1752.
”Effects of gravitational darkening on the determination of fundamental parameters in fast-rotating B-type stars”. Astronomy and Astrophysics 440 (1): sid. 305–320. september 2005. doi:10.1051/0004-6361:20042229. https://arxiv.org/abs/astro-ph/0503381.
”On the evolutionary status of Be stars. I. Field Be stars near the Sun”. Astronomy and Astrophysics 441 (1): sid. 235–248. oktober 2005. doi:10.1051/0004-6361:20053051. https://arxiv.org/abs/astro-ph/0509119.
”Spitzer 24 μm Survey of Debris Disks in the Pleiades”. The Astrophysical Journal 649 (2): sid. 1028–1042. oktober 2006. doi:10.1086/506373. https://arxiv.org/abs/astro-ph/0606039.

books.google.com

Allen, Richard Hinckley (1899). Star-names and their meanings. G. E. Stechert. sid. 406. https://books.google.com/books?id=5xQuAAAAIAAJ. Läst 10 oktober 2009

doi.org

dx.doi.org

Van Leeuwen, F. (2007). ”Validation of the new Hipparcos reduction”. Astronomy and Astrophysics 474 (2): sid. 653. doi:10.1051/0004-6361:20078357. https://arxiv.org/abs/0708.1752.
”Highly ionized stellar winds in Be stars. II - Winds in B6-B9.5e stars”. Astrophysical Journal, Part 1 339: sid. 403–419. april 1989. doi:10.1086/167306.
Zhang, P; Liu, C. Q; Chen, P. S (2006). ”Absolute Magnitudes of Be Stars Based on Hipparcos Parallaxes”. Astrophysics and Space Science 306 (3): sid. 113. doi:10.1007/s10509-006-9173-1.
”Effects of gravitational darkening on the determination of fundamental parameters in fast-rotating B-type stars”. Astronomy and Astrophysics 440 (1): sid. 305–320. september 2005. doi:10.1051/0004-6361:20042229. https://arxiv.org/abs/astro-ph/0503381.
”Lithium in Brown Dwarf Candidates: The Mass and Age of the Faintest Pleiades Stars”. Astrophysical Journal 458: sid. 600–609. 1996. doi:10.1086/176842.
”On the evolutionary status of Be stars. I. Field Be stars near the Sun”. Astronomy and Astrophysics 441 (1): sid. 235–248. oktober 2005. doi:10.1051/0004-6361:20053051. https://arxiv.org/abs/astro-ph/0509119.
”The Frequency of Spectroscopic Binaries in the Pleiades”. Astrophysical Journal 142: sid. 1604–1615. november 1965. doi:10.1086/148440.
”Four Suspected Spectroscopic Binaries in the Pleiades”. Publications of the Astronomical Society of the Pacific 83 (494): sid. 493–495. 1971. doi:10.1086/129161.
”Spitzer 24 μm Survey of Debris Disks in the Pleiades”. The Astrophysical Journal 649 (2): sid. 1028–1042. oktober 2006. doi:10.1086/506373. https://arxiv.org/abs/astro-ph/0606039.

iau.org

”IAU Working Group on Star Names (WGSN)”. International Astronomical Union. https://www.iau.org/science/scientific_bodies/working_groups/280/. Läst 22 maj 2016.

rochester.edu

pas.rochester.edu

”IAU Catalog of Star Names”. http://www.pas.rochester.edu/~emamajek/WGSN/IAU-CSN.txt. Läst 28 juli 2016.