Jump to content
 







Main menu
   


Navigation  



Main page
Contents
Current events
Random article
About Wikipedia
Contact us
Donate
 




Contribute  



Help
Learn to edit
Community portal
Recent changes
Upload file
 








Search  

































Create account

Log in
 









Create account
 Log in
 




Pages for logged out editors learn more  



Contributions
Talk
 



















Contents

   



(Top)
 


1 References  














36 Lyncis






Нохчийн
Svenska
Татарча / tatarça
Українська

 

Edit links
 









Article
Talk
 

















Read
Edit
View history
 








Tools
   


Actions  



Read
Edit
View history
 




General  



What links here
Related changes
Upload file
Special pages
Permanent link
Page information
Cite this page
Get shortened URL
Download QR code
Wikidata item
 




Print/export  



Download as PDF
Printable version
 
















Appearance
   

 






From Wikipedia, the free encyclopedia
 


36 Lyncis


Alight curve for EI Lyncis, plotted from TESS data[1]

Observation data
Epoch J2000      Equinox J2000
Constellation Lynx
Right ascension 09h13m 48.21318s[2]
Declination +43° 13′ 04.1940″[2]
Apparent magnitude (V) 5.30[3]
Characteristics
Spectral type B9IVpHgMn[4]
B−V color index −0.130±0.003[3]
Variable type SX Ari[5]
Astrometry
Radial velocity (Rv)21.3±1.7[3] km/s
Proper motion (μ) RA: –30.236[2] mas/yr
Dec.: −32.032[2] mas/yr
Parallax (π)5.2687 ± 0.1577 mas[2]
Distance620 ± 20 ly
(190 ± 6 pc)
Absolute magnitude (MV)−0.95[3]
Details
Mass4.2[2] M
Radius4.21[6] R
Luminosity505[2] L
Surface gravity (log g)3.65[7] cgs
Temperature13,700[7] K
Metallicity [Fe/H]+0.60[7] dex
Rotation3.83476±0.00004 d[8]
Rotational velocity (v sin i)49±1[8] km/s
Other designations

36 Lyn, EI Lyn, BD+43°1893, FK5 346, HD 79158, HIP 45290, HR 3652, SAO 42759[9]

Database references
SIMBADdata

36 Lyncis is a solitary[10] variable star located around 620 light years away from the Sun in the northern constellationofLynx. It has the variable star designationofEI Lyncis, while 36 Lyncis is the Flamsteed designation. This object is visible to the naked eye as a dim, blue-white hued star with an apparent visual magnitude of 5.30.[3] It is moving further away from the Earth with a heliocentric radial velocity of 21 km/s.[3]

This is a magnetic, helium-weak Bp star[11][12] with a stellar classification of B9IVpHgMn,[4] although the spectral peculiarities have led to alternate classifications such as B8 IIImnp.[8] It is sometimes classified as a mercury-manganese star.[13] It is also an 'sn' star, displaying a spectrum with generally sharp lines for most elements in combination with broad, diffuse lines of helium.[14] 36 Lyncis has been classified as an SX Arietis variable[15] with an amplitude of 0.03 in visual magnitude and a rotationally-modulated period of 3.834 days.[5] The star is spinning with a projected rotational velocity of 49 km/s[8] and a rotation rate of 3.83476 days.[8] It has 4.21[6] times the Sun's radius and is radiating 505 times the luminosity of the Sun from its photosphere at an effective temperatureof13,700 K.[7]

References

[edit]
  1. ^ "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved 8 December 2021.
  • ^ a b c d e f g Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this sourceatVizieR.
  • ^ a b c d e f Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. S2CID 119257644.
  • ^ a b Abt, Helmut A.; Morrell, Nidia I. (July 1995). "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars". The Astrophysical Journal Supplement Series. 99: 135. Bibcode:1995ApJS...99..135A. doi:10.1086/192182. ISSN 0067-0049.
  • ^ a b Samus, N. N.; et al. (2017). "General Catalogue of Variable Stars". Astronomy Reports. 5.1. 61 (1): 80–88. Bibcode:2017ARep...61...80S. doi:10.1134/S1063772917010085. S2CID 125853869.
  • ^ a b Shulyak, D.; et al. (2014). "Interferometry of chemically peculiar stars: Theoretical predictions versus modern observing facilities". Monthly Notices of the Royal Astronomical Society. 443 (2): 1629. arXiv:1406.6093. Bibcode:2014MNRAS.443.1629S. doi:10.1093/mnras/stu1259. S2CID 96452769.
  • ^ a b c d Ghazaryan, S.; et al. (November 2018). "New catalogue of chemically peculiar stars, and statistical analysis". Monthly Notices of the Royal Astronomical Society. 480 (3): 2953–2962. arXiv:1807.06902. Bibcode:2018MNRAS.480.2953G. doi:10.1093/mnras/sty1912. S2CID 119062018.
  • ^ a b c d e Cowley, A. (November 1972). "Spectral classification of the bright B8 stars". Astronomical Journal. 77: 750–755. Bibcode:1972AJ.....77..750C. doi:10.1086/111348.
  • ^ "36 Lyncis". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-06-06.
  • ^ Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869–879. arXiv:0806.2878. Bibcode:2008MNRAS.389..869E. doi:10.1111/j.1365-2966.2008.13596.x. S2CID 14878976.
  • ^ Oksala, M. E.; Silvester, J.; Kochukhov, O.; Neiner, C.; Wade, G. A.; MiMeS Collaboration (January 2018). "Mixed poloidal-toroidal magnetic configuration and surface abundance distributions of the Bp star 36 Lyn". Monthly Notices of the Royal Astronomical Society. 473 (3): 3367–3376. arXiv:1709.08361. Bibcode:2018MNRAS.473.3367O. doi:10.1093/mnras/stx2487. S2CID 4158836.
  • ^ Adelman, Saul J. (May 2000). "UVBY photometry of the magnetic CP stars HD 36668, 36 Lyncis, HD 86592, and HR 8861". Astronomy and Astrophysics. 357: 548–552. Bibcode:2000A&A...357..548A.
  • ^ Ghazaryan, S.; Alecian, G.; Hakobyan, A. A. (2018). "New catalogue of chemically peculiar stars, and statistical analysis". Monthly Notices of the Royal Astronomical Society. 480 (3): 2953–2962. arXiv:1807.06902. Bibcode:2018MNRAS.480.2953G. doi:10.1093/mnras/sty1912. S2CID 119062018.
  • ^ Shore, Steven N.; et al. (September 1987). "The SN Stars: Magnetically Controlled Stellar Winds Among the Helium-Weak Stars". Astronomical Journal. 94: 737. Bibcode:1987AJ.....94..737S. doi:10.1086/114512.
  • ^ Watson, Christopher (4 January 2010). "EI Lyncis". AAVSO Website. American Association of Variable Star Observers. Retrieved 21 October 2022.

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=36_Lyncis&oldid=1235039112"

    Categories: 
    B-type subgiants
    Helium-weak stars
    Mercury-manganese stars
    SX Arietis variables
    Lynx (constellation)
    Durchmusterung objects
    Flamsteed objects
    Henry Draper Catalogue objects
    Hipparcos objects
    Bright Star Catalogue objects
    Objects with variable star designations
    Hidden categories: 
    Articles with short description
    Short description matches Wikidata
     



    This page was last edited on 17 July 2024, at 11:50 (UTC).

    Text is available under the Creative Commons Attribution-ShareAlike License 4.0; additional terms may apply. By using this site, you agree to the Terms of Use and Privacy Policy. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc., a non-profit organization.



    Privacy policy

    About Wikipedia

    Disclaimers

    Contact Wikipedia

    Code of Conduct

    Developers

    Statistics

    Cookie statement

    Mobile view



    Wikimedia Foundation
    Powered by MediaWiki