| 释义 |
- References
{{Starbox begin
| name=36 Lyncis }}{{Starbox observe
| epoch = J2000
| ra = {{RA|09|13|48.20765}}
| dec = {{DEC|+43|13|04.1751}}
| appmag_v =
| constell = Lynx
}}{{Starbox character
| class = B8IIIp
| b-v =
| u-b =
| variable = SX Arietis variable
}}{{Starbox astrometry
| radial_v = {{Val|21.30|1.7}}
| prop_mo_ra = –27.87 ± 0.24
| prop_mo_dec = -35.46 ± 0.15
| parallax = 5.61
| p_error = 0.31
| parallax_footnote =
| absmag_bol =
}}{{Starbox detail
| mass =
| radius =
| luminosity = 2,848[6]
| gravity =
| temperature = 3,485[6]
| metal_fe =
| rotational_velocity =
| age =
}}{{Starbox catalog
| names = 36 Lyncis, EI Lyncis, BD +43 1893, FK5 346, HD 79158, HR 3652, HIP 45290, SAO 42759.[8]
}}{{Starbox reference|Simbad=36+Lyn}}{{Starbox end}}36 Lyncis, also known by its variable star designation of EI Lyncis, is a star in the constellation Lynx. It is a blue giant of spectral type B8III. It has been classified as an SX Arietis variable.[1] Located around 580 light-years distant, it shines with a luminosity approximately 325 times that of the Sun and has a surface temperature of 11,644 K.[6] References 1. ^{{cite web|url=http://www.aavso.org/vsx/index.php?view=detail.top&oid=136468 |title=EI Lyncis |author=Watson, Christopher |date=4 January 2010 |work=AAVSO Website|publisher=American Association of Variable Star Observers|accessdate=20 March 2016}}
2. ^1 2 3 {{cite journal | display-authors=1 | last1=McDonald | first1=I. | last2=Zijlstra | first2=A. A. | last3=Boyer | first3=M. L. | title=Fundamental Parameters and Infrared Excesses of Hipparcos Stars | journal=Monthly Notices of the Royal Astronomical Society | volume=427 | issue=1 | pages=343–57 | date=2012 | bibcode=2012MNRAS.427..343M | arxiv=1208.2037 | doi=10.1111/j.1365-2966.2012.21873.x }}
3. ^1 {{cite simbad | title=36 Lyncis | accessdate=20 March 2016}}
}}{{Stars of Lynx}}{{giant-star-stub}} 9 : Lynx (constellation)|SX Arietis variables|B-type giants|Flamsteed objects|Hipparcos objects|HR objects|Henry Draper Catalogue objects|Objects with variable star designations|Durchmusterung objects |