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University of Illinois at Urbana-Champaign

Molecular gas in S106: Morphology, kinematics, and chemistry of a star-forming region

Abstract

dc:description

The biconical H II region S106 is a site of recent star formation; it consists of two ionized lobes flowing out from a central disk of cold molecular gas in which is embedded the newly formed massive star IRS 4. This entire complex is still embedded in the molecular cloud from which it formed.

Degree

thesis:*
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
2011

Author and committee

dc:creator, dc:contributor.*
Author dc:creator
  • Loushin, Robert Stephen
Contributors dc:contributor
  • Webbink, Ronald F.

Subjects

dc:subject × 1

Rights

dc:rights
Statement dc:rights
  • Copyright 1989 Loushin, Robert Stephen
Language dc:language
eng

Identifiers

dc:identifier.*
Identifier
AAI9010941
(UMI)AAI9010941
OAI identifier oai:identifier
oai:www.ideals.illinois.edu:2142/20374

Chain of custody

source
Harvested from
University of Illinois - Urbana-Champaign
Base URL
www.ideals.illinois.edu/oai-pmh
Last updated
2026-07-22
Source record
OAI-PMH GetRecord
citation

Loushin, Robert Stephen. Molecular gas in S106: Morphology, kinematics, and chemistry of a star-forming region. Dissertation thesis, University of Illinois at Urbana-Champaign, 2011. http://hdl.handle.net/2142/20374