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A connection between the rate of rotation of interstellar clouds, magnetic fields, ambipolar diffusion, and the periods of binary stars

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/154912· OSTI ID:7130644
Observations do not show any interstellar clouds rotating much faster than the Galaxy. This can be attributed to magnetic braking, which the observed parameters of the interstellar medium show to be very efficient as long as the magnetic field is frozen in the matter. The critical density n/sub cr/ at which the field decouples from the matter determines the period of rotation of a binary star system, assumed to form by a collapsing (nearly nonmagnetic) fragment that conserves its angular momentum. The observed periods tau/sub b/ of binary stars (roughly 100 yr > or approx. = tau/sub b/> or approx. = 10 hr) may be accounted for if n/sub cr/ ranges from 7.5 x 10/sup 3/ cm/sup -3/ to 2.2 x 10/sup 6/ cm/sup -3/, respectively. We reexamine the process of ambipolar diffusion (by appropriately scaling the field strength to dense-cloud densities) and show that, at the above densities, it can decouple the field from the matter within 8.8 x 10/sup 5/ to 3.9 x 10/sup 7/ years. A scenario for star formation is outlined. (AIP)
Research Organization:
Department of Astrophysical Sciences, Princeton University
OSTI ID:
7130644
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 211:1; ISSN ASJOA
Country of Publication:
United States
Language:
English