Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-23T19:00:29.444Z Has data issue: false hasContentIssue false
  • English
  • Français

IR Line and Continuum Emission from Bipolar Outflow Sources

Published online by Cambridge University Press:  04 August 2017

Howard A. Smith ,
J. Fischer ,
D. Mozurkewich ,
P. R. Schwartz  and
T. R. Geballe
Howard A. Smith
Affiliation:
Naval Research Lab. Code 4139.5, Washington, DC 20375 USA
J. Fischer
Affiliation:
Naval Research Lab. Code 4139.5, Washington, DC 20375 USA
D. Mozurkewich
Affiliation:
Naval Research Lab. Code 4139.5, Washington, DC 20375 USA
P. R. Schwartz
Affiliation:
Naval Research Lab. Code 4139.5, Washington, DC 20375 USA
T. R. Geballe
Affiliation:
UKIRT, 665 Komohama St., Hilo, HI 96720, USA

Extract

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.

Most of our understanding of BPF's is based on observations of the neutral and ionized gas in bright, high luminosity sources. Data on low luminosity (L ≲ 30 L⊙) objects has now become more available (e.g. Frerking and Langer, Astrophys. J. 256, 523, 1982) permitting a test of models at this end of the luminosity range. We have performed a series of multi-wavelength observations, emphasizing low luminosity objects.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 343 - 345
Copyright
Copyright © Reidel 1987