Formation Rate of Triple Stars relative to Double Stars

Details Formation Rate of Triple Stars relative to Double Stars Formation Rate of Triple Stars relative to Double Stars

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..491i&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 491-492

Astronomy and Astrophysics

Astrophysics

1

Triple Stars, Circumstellar Envelope, Speckle Observations

Scientific paper

A series of our and McAlisteret al.'s speckle observations of spectroscopic binaries show that certain fractions of them are triple systems. A typical configuration of those systems is that of two stars separated by about 0.1 AU with a third component in an orbit at a distance about 10 AU from the central stars. These results suggest that the third star was formed from the outer circumstellar envelope after forming the central double.

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