No CrossRef data available.
Article contents
Infrared Jets from Protostars: The case of HH212
Published online by Cambridge University Press: 12 April 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
We describe the appearance and significance of HH212, the most symmetric two-sided molecular hydrogen jet/counterjet system yet discovered. This prototype embedded protostellar H2 jet emanates from a low-luminosity isolated protostar in Orion. It exhibits matched pairs of knots and bow-shocks interpreted as arising from a time-variable source, which we take to indicate that protostellar accretion through the encircling disk is non-steady and pulsed.
- Type
- Part 11. Young Stellar Objects
- Information
- International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 531 - 535
- Copyright
- Copyright © Astronomical Society of the Pacific 1997
References
Bally, J., Morse, J., & Reipurth, B.
1996, in Science with the Hubble Space Telescope—II, eds. Benvenuti, P., Macchetto, F.D., & Schreier, E.J., p 491
Google Scholar
Reipurth, B., 1994, A General Catalog of Herbig-Haro Objects, electronically published via anonymous ftp at ftp.hq.eso.org, directory pub/Catalogs/Herbig-HaroGoogle Scholar
Zinnecker, H., McCaughrean, M.J., & Rayner, J.T.
1996, in Disks and Outflows around Young Stars, eds. Beckwith, S., Staude, J., Quetz, A., & Natta, A., Lecture Notes in Physics
465, (Heidelberg: Springer), p 236
Google Scholar
You have
Access