On the possibility of outflows from very low-mass companions

Details On the possibility of outflows from very low-mass companions On the possibility of outflows from very low-mass companions

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pasp..102..745w&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 102, July 1990, p. 745-748.

Astronomy and Astrophysics

Astrophysics

9

Companion Stars, Stellar Mass Ejection, Binary Stars, Missing Mass (Astrophysics), Pre-Main Sequence Stars, Stellar Luminosity

Scientific paper

High-velocity outflows, once thought to be possible only for massive pre-main-sequence stars, have been found associated with sources of less than solar mass. The possibility that even much smaller objects may, at some stage of their early lives, drive such outflows is investigated. The predicted properties of outflows from these low-mass objects are such that they would be very difficult to detect directly. If, however, the low-mass source is the companion of a larger star the outflow may have interesting and possibly detectable effects on the development of the combined system.

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