Kang, 98 Virginis, κ Vir, BD−09°3878, FK5 523, HD 124294, HIP 69427, HR 5315, SAO 158427[7]
Database references
SIMBAD
data
Kappa Virginis (κ Virginis, abbreviated Kappa Vir, κ Vir), officially named Kang/ˈkæŋ/,[8] is a solitary star in the zodiac constellation of Virgo. It has an apparent visual magnitude of 4.18,[2] which is sufficiently bright to be seen with the naked eye. Based upon stellar parallax measurements, the distance to this star is about 255 light-years.
^ abcdeCite error: The named reference van Leeuwen2007 was invoked but never defined (see the help page).
^ abcdCite error: The named reference Jennens1975 was invoked but never defined (see the help page).
^Cite error: The named reference Houk1999 was invoked but never defined (see the help page).
^ abCite error: The named reference Massarotti2008 was invoked but never defined (see the help page).
^Cite error: The named reference Anderson2012 was invoked but never defined (see the help page).
^ abcdefgCite error: The named reference Villaver2013 was invoked but never defined (see the help page).
^Cite error: The named reference SIMBAD was invoked but never defined (see the help page).
^"Naming Stars". IAU.org. Retrieved 16 December 2017.
KappaVirginis (κ Virginis, abbreviated Kappa Vir, κ Vir), officially named Kang /ˈkæŋ/, is a solitary star in the zodiac constellation of Virgo. It has...
Iota Virginis (ι Virginis, abbreviated Iota Vir, ι Vir) is a binary star in the constellation of Virgo. Its apparent magnitude is 4.08. Based on its parallax...
gangs in the "Paradise Towers" 1987 Doctor Who episode Kang, the star KappaVirginis Kang bed-stove K'ang jo fu or the kang, a self-defense technique KANG-LD...
Lambda Virginis (λ Virginis, abbreviated Lambda Vir, λ Vir) is a binary star system in the zodiac constellation of Virgo. With an apparent visual magnitude...
Phi Virginis (φ Virginis, abbreviated Phi Vir, φ Vir) is a binary star in the zodiac constellation of Virgo. It can be seen with the naked eye, having...
from about 30 min down to about 1 minute. GW Virginis and ZZ Ceti stars are thought to be excited by the kappa mechanism; V777 Herculis stars by convective...
Kappa Pavonis (κ Pav) is a variable star in the constellation Pavo. It is the brightest W Virginis variable in the sky. In 1901, κ Pavonis was reported...
Star Slightly variable 3.38 3.32 Delta Virginis Star 3.38 Epsilon Hydrae Quintuple star system 3.38 Zeta Virginis Binary star system Slightly variable 3...
between 1 and 4 days are of the BL Her subclass, 10–20 days belong to the W Virginis subclass, and stars with periods greater than 20 days belong to the RV...
galaxies NGC 5128 and NGC 4258. Historically Type II Cepheids were called W Virginis variables, but are now divided into three subclasses based on the length...
Cambridge University Press. p. 170. ISBN 0-521-44921-9. Kaler, James B. "Saiph (Kappa Orionis)". Stars. University of Illinois. Archived from the original on...
to the near absence of repetitiveness in the irregular variables. The W Virginis variables are at the interface; the short period ones are regular and the...
five stars, the largest depicting Sirius Canopus (α Carinae) Spica (α Virginis) Hydra: two stars, the larger being Alphard Crux Australis: five stars...
flanked by two towers holding above a banner with the Latin words "Civitas Virginis") surrounded by the collar of the Order of the Tower and Sword and topped...
Angle of the Barking Dog زاوية العواء Beta Virginis Zawiah aka Zaniah az-Zāwiyah The angle الزاوية Eta Virginis Zubenelgenubi az-Zubān ul-Janūbiy Southern...
Women Ad tuendam fidem Novo millennio ineunte Misericordia Dei Rosarium Virginis Mariae The Rapid Development Encyclicals Redemptor hominis Dives in misericordia...
Wall Gamma Virginis Porrima 東上相 Dōng Shàng Xiàng The First Eastern Minister 太微左垣三 Tài Wēi Zuǒ Yuán sān the Third Star of Left Wall Delta Virginis Minelauva...
L. (1986). "Heavy-element abundances in the mild barium stars Omicron Virginis and 16 Serpentis". The Astrophysical Journal. 311: 819. Bibcode:1986ApJ...
acronym BCEPS. The pulsations of Beta Cephei variables are driven by the kappa mechanism and p-mode pulsations. At a depth within the star where the temperature...
companions to post-common envelope binaries. III. A reexamination of HW Virginis". Astronomy & Astrophysics. 543: id.A138. arXiv:1206.3080. Bibcode:2012A&A...
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