First Image with the CfA Superconductive HEB Receiver: The Protostellar Outflow from IRAS 20126+4104 in CO ( \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $J=7$ \end{document} –6)

Journal article published in 1999 by J. H. Kawamura, T. R. Hunter , C.‐Y E. Tong, R. Blundell, Q. Zhang , C. A. Katz, D. C. Papa, T. K. Sridharan

This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

Preprint: archiving allowed

Upload

Postprint: archiving allowed

Upload

Published version: archiving forbidden

Policy details

Data provided by