Orion B--Anatomy of a Star-Forming Region
type: CreativeWork
description: 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 $\mu$m, and in several millimeter-wavelength molecular transitions (of HCO$\sp+$, SO, H$\sp $CN, and HC$\sp $N) with the Hat Creek Array.
abstract: The compact HII region/molecular cloud Orion B was observed with the VLA in the radio continuum and OH absorption line at a frequency of 1667 MHz, in the near-infrared continuum and H$\sb2$ emission line at a wavelength of 2 $\mu$m, and in several millimeter-wavelength molecular transitions (of HCO$\sp+$, SO, H$\sp $CN, and HC$\sp $N) with the Hat Creek Array.
author: Barnes, Peter John
keywords: Physics, Astronomy and Astrophysics
date published: 2014-12-16T00:55:18Z
date modified: 2026-07-22T22:26:03Z
provider: University of Illinois - Urbana-Champaign
publisher: Networked Digital Library of Theses and Dissertations
type: WebPage
source organization: University of Illinois at Urbana-Champaign

PropertyValue
property ID: Handle
value: http://hdl.handle.net/2142/70671