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Title: CO emission structure in the Taurus molecular cloud complex

Abstract

A survey of the J = 1 0 2.6 mm transition of CO covering 11.5 degS toward the Taurus dark cloud complex reveals three indications of systematic velocity structure:

Authors:
;
Publication Date:
Research Org.:
Research Laboratory of Electronics and Department of Physics, Massachusetts Institute of Technology
OSTI Identifier:
6328709
Resource Type:
Journal Article
Journal Name:
Astrophys. J.; (United States)
Additional Journal Information:
Journal Volume: 298:2
Country of Publication:
United States
Language:
English
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; CARBON MONOXIDE; EMISSION; INTERSTELLAR GRAINS; ENERGY-LEVEL TRANSITIONS; MAPS; MASS; NEBULAE; STELLAR WINDS; T TAURI STARS; CARBON COMPOUNDS; CARBON OXIDES; CHALCOGENIDES; ERUPTIVE VARIABLE STARS; OXIDES; OXYGEN COMPOUNDS; PARTICLES; STARS; STELLAR ACTIVITY; VARIABLE STARS; 640105* - Astrophysics & Cosmology- Galaxies

Citation Formats

Murphy, D.C., and Myers, P.C. CO emission structure in the Taurus molecular cloud complex. United States: N. p., 1985. Web. doi:10.1086/163663.
Murphy, D.C., & Myers, P.C. CO emission structure in the Taurus molecular cloud complex. United States. doi:10.1086/163663.
Murphy, D.C., and Myers, P.C. Fri . "CO emission structure in the Taurus molecular cloud complex". United States. doi:10.1086/163663.
@article{osti_6328709,
title = {CO emission structure in the Taurus molecular cloud complex},
author = {Murphy, D.C. and Myers, P.C.},
abstractNote = {A survey of the J = 1 0 2.6 mm transition of CO covering 11.5 degS toward the Taurus dark cloud complex reveals three indications of systematic velocity structure:},
doi = {10.1086/163663},
journal = {Astrophys. J.; (United States)},
number = ,
volume = 298:2,
place = {United States},
year = {1985},
month = {11}
}