Dorrit Hoffleit

“Science capital”: A conceptual, methodological, and empirical argument for extending bourdieusian notions of capital beyond the arts

Energy input from quasars regulates the growth and activity of black holes and their host galaxies

Dust in Starburst Galaxies

Gravitational Collapse and Space-Time Singularities

A Probability Theory of Cluster Analysis

On the nature of quasars and active galactic nuclei

The Dust Content and Opacity of Actively Star‐forming Galaxies

Cosmic Discovery: The Search, Scope and Heritage of Astronomy

Improving the rate of success for underrepresented racial minorities in STEM fields: Insights from a national project

A Simple Model for the Absorption of Starlight by Dust in Galaxies

Barriers to Faculty Pedagogical Change: Lack of Training, Time, Incentives, and…Tensions with Professional Identity?

“Doing” science versus “being” a scientist: Examining 10/11‐year‐old schoolchildren's constructions of science through the lens of identity

Supermassive Black Holes in Galactic Nuclei: Past, Present and Future Research

What are we doing here? Analyzing fifteen years of energy scholarship and proposing a social science research agenda

Antimatter, Quasi-stellar Objects, and the Evolution of Galaxies

An Analysis of the Shapes of Interstellar Extinction Curves. VII. Milky Way Spectrophotometric Optical-through-ultraviolet Extinction and Its R-dependence*

Mission Concept for the Single Aperture Far-Infrared (SAFIR) Observatory

Gravitational Collapse

Relativistic Astrophysics

On Two Theories of the Cyclical Outbursts of η Carinae

Massive Stars, Relativistic Polytropes, and Gravitational Radiation

What are we talking about when we talk about STEM education? A review of literature

A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s⁻¹ Mpc⁻¹ Uncertainty from the Hubble Space Telescope and the SH0ES Team

Industrial market segmentation by the structure of the purchasing process

GG Tauri's Circumbinary Disk: Models for Near‐Infrared Scattered‐Light Images and¹³CO ( \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 $J=1arrow 0$ \end{document} ) Line Profiles

Rethinking gender and identity in energy studies

Understanding the science experiences of successful women of color: Science identity as an analytic lens

The Angular Diameters of 32 Stars

The Pistol Star

Quasi-Stellar Sources: Variation in the Radio Emission of 3C 273

THEM-σ ANDM-LRELATIONS IN GALACTIC BULGES, AND DETERMINATIONS OF THEIR INTRINSIC SCATTER

The Bright Star Catalogue, 5 th revised edition.

Catalogue of Bright Stars

Distances for Southern Early-Type Stars, Especially in Carina and Other H II Regions.

Light Variability and Nature of 3C273.

Light Variations in the Superluminous Radio Galaxy 3C273