Orion B--Anatomy of a Star-Forming Region

The compact HII region/molecular cloud Orion B was observed with the VLA in the radio continuum and OH absorption line at a frequency of 1667 MHz, in the near-infrared continuum and H$\sb2$ emission line at a wavelength of 2 μm, and in several millimeter-wavelength molecular transitions (of HCO$\sp+$, SO, H$\sp $CN, and HC$\sp $N) with the Hat Creek Array.

Name thesis:degree_name

Ph.D.

Level thesis:degree_level

Dissertation

Discipline thesis:degree_discipline

Astronomy

Grantor

University of Illinois at Urbana-Champaign

Year dc:date

2014

Author dc:creator

• Barnes, Peter John

Contributors dc:contributor

• Crutcher, Richard M.

• Physics, Astronomy and Astrophysics

Identifier

(UMI)AAI8908619

OAI identifier oai:identifier

oai:www.ideals.illinois.edu:2142/70671