Neal Evans
0000-0001-5175-1777
University of California
494 papers found
Refreshing results…
The BIMA Survey of Embedded Cores in the Perseus Cloud Complex
The Physical Conditions for Massive Star Formation: Dust Continuum Maps and Modeling
CS J=7-6 Mapping of Massive Star Formation Regions Associated with Water Masers
Probing the Birth of Hot Cores through Mid-Infrared and Submillimeter Spectroscopy of HCN and C2H2
Dust Continuum Observations of Massive Star Forming Regions
OB Star Forming Clouds: Physical Conditions on Large Scales
A CS J=5-4 Mapping Survey Towards High Mass Star-Forming Cores Associated with H2O Masers
Dust and Molecular Emission from the S235 Star Forming Region
The Formation and Early Evolution of Massive Stars
Tracing the Mass during Low‐Mass Star Formation. III. Models of the Submillimeter Dust Continuum Emission from Class 0 Protostars
Initial Conditions for Star Formation
Formation of Substellar Objects: A SIRTF Legacy
The Velocity Structures in Protostellar Cores
Photon‐dominated Regions in Low‐Ultraviolet Fields: A Study of the Peripheral Region of L1204/S140
Observations of H \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 $^{+}_{3}$ \end{document} in the Diffuse Interstellar Medium
Probing the Invisible Universe: The Case for Far-IR/Submillimeter Interferometry
Observations of Infrared Molecular Lines Toward the Massive Protostar GL 2591
Modeling the Submillimeter Dust Continuum Emission from Nearby Low Mass Star Forming Cores
Tracing the Mass in Low-Mass Star Formation: Preprotostellar to Class I Cores
Tracing the Mass during Low‐Mass Star Formation. II. Modeling the Submillimeter Emission from Preprotostellar Cores
Missing publications? Search for publications with a matching author name.