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)
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
Similar Records
Ambipolar diffusion in interstellar clouds: one-dimensional, isothermal collapse
Numerical study of the effects of ambipolar diffusion on the collapse of magnetic gas clouds
Magnetic braking of self-gravitating, oblate interstellar clouds
Thesis/Dissertation
·
Fri Dec 31 23:00:00 EST 1982
·
OSTI ID:5073071
Numerical study of the effects of ambipolar diffusion on the collapse of magnetic gas clouds
Journal Article
·
Tue Dec 14 23:00:00 EST 1982
· Astrophys. J.; (United States)
·
OSTI ID:6214088
Magnetic braking of self-gravitating, oblate interstellar clouds
Journal Article
·
Wed Feb 14 23:00:00 EST 1979
· Astrophys. J.; (United States)
·
OSTI ID:5929189
Related Subjects
640102 -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
640105* -- Astrophysics & Cosmology-- Galaxies
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
AMBIPOLAR DIFFUSION
ANGULAR MOMENTUM
ANGULAR VELOCITY
BINARY STARS
COSMIC GASES
COSMIC RADIO SOURCES
DIFFUSION
FLUIDS
GASES
H1 REGIONS
INTERSTELLAR MAGNETIC FIELDS
INTERSTELLAR SPACE
MAGNETIC FIELDS
MOTION
ROTATION
SPACE
STAR ACCRETION
STAR EVOLUTION
STARS
VELOCITY
Radio & X-Ray Sources
640105* -- Astrophysics & Cosmology-- Galaxies
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
AMBIPOLAR DIFFUSION
ANGULAR MOMENTUM
ANGULAR VELOCITY
BINARY STARS
COSMIC GASES
COSMIC RADIO SOURCES
DIFFUSION
FLUIDS
GASES
H1 REGIONS
INTERSTELLAR MAGNETIC FIELDS
INTERSTELLAR SPACE
MAGNETIC FIELDS
MOTION
ROTATION
SPACE
STAR ACCRETION
STAR EVOLUTION
STARS
VELOCITY