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 See also  





2 References  














HD 93403






עברית
Svenska
 

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
 


HD 93403
Observation data
Epoch J2000      Equinox J2000
Constellation Carina
Right ascension 10h45m 44.11931s[1]
Declination −59° 24′ 28.1431″[1]
Apparent magnitude (V) 7.272[2]
Characteristics
Spectral type O5.5III(fc)var[3] (O5.5I + O7V[4])
U−B color index −0.747[2]
B−V color index +0.212[2]
Astrometry
Radial velocity (Rv)14.80 km/s
Proper motion (μ) RA: -7.27 mas/yr
Dec.: 2.45 mas/yr
Parallax (π)1.22 ± 0.45 mas[1]
Distance3,200[4] pc
Orbit[5]
Period (P)15.093 days
Semi-major axis (a)121 R
Eccentricity (e)0.234
Inclination (i)~31°
Semi-amplitude (K1)
(primary)
79.3 km/s
Semi-amplitude (K2)
(secondary)
139.0 km/s
Details[4]
Primary
Mass68.5[5] M
Radius24 R
Luminosity1,050,000 L
Temperature39,300 K
Secondary
Mass37.3[5] M
Radius10 R
Luminosity257,000 L
Temperature40,100 K
Other designations

HD 93403, HIP 52628, CD−58°3545, 2MASS J10454411-5924281, GSC 08626-00641, TYC 8626-641-1

Database references
SIMBADdata

HD 93403 is a spectroscopic binary containing two highly luminous hot blue stars. It is 10,000 light years away in the Carina Nebula in the constellation Carina. It appears to have spectral type O5.5III, but this is composed of two spectra from a blue supergiant and blue main sequence star of spectral type O5.5I and O7V respectively. The two stars orbit every 15 days with a separation that varies from 93 R to 149 R. The binary is shedding mass at the high rate of 0.0005 M per year.[3]

HD 93403 exhibits the Struve-Sahade effect, where the strength of the spectral lines of the individual components varies during the orbit. It also has colliding stellar winds that produce variable x-ray[6] and non-thermal radio emission.[7]

See also

[edit]

References

[edit]
  1. ^ a b c van Leeuwen, Floor (13 August 2007). "Validation of the new Hipparcos reduction". Astronomy & Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. eISSN 1432-0746. ISSN 0004-6361.
  • ^ a b c Maíz-Apellániz, Jesús; Walborn, Nolan R.; Galué, Héctor Á.; Wei, Lisa H. (2004). "A Galactic O Star Catalog". The Astrophysical Journal Supplement Series. 151 (1): 103–148. arXiv:astro-ph/0311196. Bibcode:2004ApJS..151..103M. doi:10.1086/381380. S2CID 118813863.
  • ^ a b Sota, A.; Maíz Apellániz, J.; Morrell, N. I.; Barbá, R. H.; Walborn, N. R.; Gamen, R. C.; Arias, J. I.; Alfaro, E. J. (2014). "The Galactic O-Star Spectroscopic Survey (GOSSS). II. Bright Southern Stars". The Astrophysical Journal Supplement Series. 211 (1): 84. arXiv:1312.6222. Bibcode:2014ApJS..211...10S. doi:10.1088/0067-0049/211/1/10. S2CID 118847528. 10.
  • ^ a b c Rauw, G.; Vreux, J.-M.; Stevens, I. R.; Gosset, E.; Sana, H.; Jamar, C.; Mason, K. O. (2002). "Phase-resolved X-ray and optical spectroscopy of the massive binary HD 93403". Astronomy and Astrophysics. 388 (2): 552. Bibcode:2002A&A...388..552R. doi:10.1051/0004-6361:20020523.
  • ^ a b c Rauw, G.; Sana, H.; Gosset, E.; Vreux, J.-M.; Jehin, E.; Parmentier, G. (2000). "A new orbital solution for the massive binary system HD 93403". Astronomy and Astrophysics. 360: 1003. Bibcode:2000A&A...360.1003R.
  • ^ Analysis of the X-ray emission of OB stars: O stars
  • ^ Palate, M.; Rauw, G.; Koenigsberger, G.; Moreno, E. (2013). "Spectral modelling of massive binary systems". Astronomy & Astrophysics. 552: A39. arXiv:1302.5201. Bibcode:2013A&A...552A..39P. doi:10.1051/0004-6361/201219754. S2CID 54771449.

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=HD_93403&oldid=1172494181"

    Categories: 
    Carina (constellation)
    Carina Nebula
    Henry Draper Catalogue objects
    O-type supergiants
    O-type main-sequence stars
    2MASS objects
    Hipparcos objects
    Emission-line stars
    Durchmusterung objects
    Spectroscopic binaries
    Hidden categories: 
    Articles with short description
    Short description is different from Wikidata
     



    This page was last edited on 27 August 2023, at 12:48 (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