Pre-main-sequence Binary Stars

Details Pre-main-sequence Binary Stars Pre-main-sequence Binary Stars

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000eaa..booke2384m&link_type=abstract

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 2384. Bristol: Institute of Physics Publishing, 2001

Astronomy and Astrophysics

Astrophysics

Stars, Binary Stars

Scientific paper

The typical product of the STAR FORMATION process is a multiple star system, most commonly a BINARY STAR. A pre-main-sequence (PMS) binary star is a pair in which, typically, both stars have not yet fully contracted to the main sequence and are not yet fusing hydrogen at their cores. Such binary stars are recently formed, with usual ages of less than 10 million years. Since stellar contraction ti...

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