Rho Persei: Perbedaan antara revisi

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Baris 99:
<ref name=mnras355_2_601>{{citation | last1=Yeşilyaprak | first1=C. | last2=Aslan | first2=Z. | title=Period-luminosity relation for M-type semiregular variables from Hipparcos parallaxes | journal=[[Monthly Notices of the Royal Astronomical Society]] | volume=355 | issue=2 | pages=601–607 |date=December 2004 | doi=10.1111/j.1365-2966.2004.08344.x | bibcode=2004MNRAS.355..601Y }}</ref>
 
<ref name=allen_tse_516>{{citation | last1=Cox | first1=Arthur N. | last2=Becker | first2=Stephen A. | last3=Pesnell | first3=W. Dean | chapter=Chapter 20. Theoretical Stellar Evolution | page=516 | title=Allen's astrophysical quantities | edition=4th | isbn=0-387-98746-0 | publisher=Springer | publication-place=New York | url=http://extras.springer.com/2000/978-0-387-95189-8/BookChap/book20.pdf | accessdate=2012-01-25 | archive-date=2016-03-04 | archive-url=https://web.archive.org/web/20160304044047/http://extras.springer.com/2000/978-0-387-95189-8/BookChap/book20.pdf | dead-url=yes }} See table 20.5</ref>
 
<ref name=SIMBAD>{{citation | title=rho Per -- Semi-regular pulsating Star | work=SIMBAD | publisher=Centre de Données astronomiques de Strasbourg | url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Rho+Persei | accessdate=2012-01-24 }}</ref>