Jets from young stars - Estimates of their physical parameters

Details Jets from young stars - Estimates of their physical parameters Jets from young stars - Estimates of their physical parameters

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986cajph..64..407m&link_type=abstract

(Conference on Jets from Stars and Galaxies, Toronto, Canada, June 24-27, 1985) Canadian Journal of Physics (ISSN 0008-4204), vo

Physics

62

Early Stars, Jet Flow, Stellar Mass Ejection, Flow Velocity, Gas Density, Herbig-Haro Objects, Mach Number, Molecular Clouds

Scientific paper

On the basis of existing observational data, the characteristic values of the physical parameters of jets from young stellar objects are estimated. The results of these estimates are as follows: velocities = 200 - 400 km/s, Mach numbers = 10 - 40, hydrogen-number densities = 15 - 150 cm-3, and mass fluxes = 10-10 - 10-7M_sun;/year. The derived Mach numbers imply reasonable jet temperatures (≈104K), being consistent with the observed emission-line spectrum. The estimated jet densities are in agreement with the idea that some high-velocity Herbig-Haro objects (v ≈ 200 km/s) represent the working surface of a freely expanding jet boring through the outer, tenuous parts of a molecular cloud.

Affiliated with

Also associated with

No associations

Rating

Jets from young stars - Estimates of their physical parameters does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Jets from young stars - Estimates of their physical parameters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Jets from young stars - Estimates of their physical parameters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1102138