Astrophysics (Index)About

WR 140

(HD 193793, V1687 Cyg)
(Wolf-Rayet star that produces much dust)

WR 140 is a Wolf-Rayet star that is the binary companion of an O-type star, the two forming a spectroscopic binary. The pair is of interest as a colliding-wind binary, a binary pair between which stellar winds collide producing shock and creating substantial dust. Characteristics of the pair:

WR 140 specific characteristics:

The companion, which has spectral type O5, is larger, brighter, and more massive, but interest in the binary is due to the Wolf Rayet star, which gives them a Wolf-Rayet-specific spectral signature.


(star,variable star)
Further reading:
https://en.wikipedia.org/wiki/WR_140
https://en.wikipedia.org/wiki/Colliding-wind_binary
http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=WR+140
https://www.roe.ac.uk/~pmw/Wr140int.htm
https://ui.adsabs.harvard.edu/abs/2011BSRSL..80..595W/abstract
RedshiftParsecs
/Distance
Lightyears
/Lookback Years
  
~01.72kpc5.61klyWR 140
Coordinates:WR 140
J202027.97608+435116.2802

Referenced by page:
stellar designation

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