D. Massa

Stellar and wind properties of massive stars in the central parsec of the Galaxy

The most massive stars in the Arches cluster

Properties of WNh stars in the Small Magellanic Cloud: evidence for homogeneous evolution

The complex, variable near-infrared extinction towards the Nuclear Bulge

Optical performance of frequency-selective bolometers

Perfect Metamaterial Absorber

A gas cloud on its way towards the supermassive black hole at the Galactic Centre

PROPER MOTIONS OF THE ARCHES CLUSTER WITH KECK LASER GUIDE STAR ADAPTIVE OPTICS: THE FIRST KINEMATIC MASS MEASUREMENT OF THE ARCHES

Evolutionary Stellar Population Synthesis at 2 A Spectral Resolution

PHYSICS OF THE GALACTIC CENTER CLOUD G2, ON ITS WAY TOWARD THE SUPERMASSIVE BLACK HOLE

The Galactic Center massive black hole and nuclear star cluster

THE GALACTIC CENTER CLOUD G2 AND ITS GAS STREAMER

COBEFar Infrared Absolute Spectrophotometer Observations of Galactic Lines

Dust in Starburst Galaxies

Late‐Time Observations of SN 2006gy: Still Going Strong

Comparison of theCOBEFIRAS and DIRBE Calibrations

Interstellar Extinction and Polarization in the Taurus Dark Clouds: The Optical Properties of Dust near the Diffuse/Dense Cloud Interface

Medium-resolution Isaac Newton Telescope library of empirical spectra

Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds

SPIFFI Observations of the Starburst SMM J14011+0252:Already Old, Fat, and Rich by z =2.565

COJ= 1-0 SPECTROSCOPY OF FOUR SUBMILLIMETER GALAXIES WITH THE ZPECTROMETER ON THE GREEN BANK TELESCOPE

Kinematics of Galaxies in the Hubble Deep Field–South: Discovery of a Very Massive Spiral Galaxy atz= 0.6

Resolved Molecular Gas and Star Formation Properties of the Strongly Lensed z = 2.26 Galaxy SDSS J0901+1814

Calibrator Design for theCOBEFar‐Infrared Absolute Spectrophotometer (FIRAS)

The Mid‐Infrared Spectrum of Star‐forming Galaxies: Global Properties of Polycyclic Aromatic Hydrocarbon Emission

High‐Redshift Supernova Rates

Optical properties of spheroidal particles

Winds from Hot Stars

Starburst‐like Dust Extinction in the Small Magellanic Cloud

Reversible Basal Plane Hydrogenation of Graphene

On the Nature of the Fast-Moving Star S2 in the Galactic Center

First-principles study of the structural and energetic properties of H atoms on a graphite () surface

Evidence for a Long‐standing Top‐heavy Initial Mass Function in the Central Parsec of the Galaxy

Infrared Emission from Interstellar Dust. II. The Diffuse Interstellar Medium

Interstellar Dust and Extinction

A BACKWARD EVOLUTION MODEL FOR INFRARED SURVEYS: THE ROLE OF AGN– AND COLOR–L_TIRDISTRIBUTIONS

The Hubble Constant: A Summary of theHubble Space TelescopeProgram for the Luminosity Calibration of Type Ia Supernovae by Means of Cepheids

Carbon onions produced by heat treatment of carbon soot and their relation to the 217.5 nm interstellar absorption feature

THE INTRINSIC TWO-DIMENSIONAL SIZE OF SAGITTARIUS A*

Photometric Stellar Variability in the Galactic Center

LINE DERIVED INFRARED EXTINCTION TOWARD THE GALACTIC CENTER

The Near-Infrared Extinction Law and Limits on the Pre–Main-Sequence Population of the ρ Ophiuchi Dark Cloud

A Reanalysis of the Ultraviolet Extinction from Interstellar Dust in the Large Magellanic Cloud

Nanostructured Plasmonic Sensors

PANCHROMATIC OBSERVATIONS AND MODELING OF THE HV TAU C EDGE-ON DISK

DISKS IN THE ARCHES CLUSTER—SURVIVAL IN A STARBURST ENVIRONMENT

NICMOS Images of the GG Tauri Circumbinary Disk

Correcting for the Effects of Interstellar Extinction

Toward a New Geometric Distance to the Active Galaxy NGC 4258. I. VLBI Monitoring of Water Maser Emission

Spatially Resolved Observations of the Galactic Center Source IRS 21

A REDETERMINATION OF THE HUBBLE CONSTANT WITH THEHUBBLE SPACE TELESCOPEFROM A DIFFERENTIAL DISTANCE LADDER

New Cepheid Period-Luminosity Relations for the Large Magellanic Cloud: 92 Near-Infrared Light Curves

Broad Family of Carbon Nanoallotropes: Classification, Chemistry, and Applications of Fullerenes, Carbon Dots, Nanotubes, Graphene, Nanodiamonds, and Combined Superstructures

Graphite, Tubular PAHs, and the Diffuse Interstellar Bands

The Distance to the Large Magellanic Cloud from the Eclipsing Binary HV 2274

Defective Carbon Onions in Interstellar Space as the Origin of the Optical Extinction Bump at 217.5 Nanometers

The Optical Properties of Metal Nanoparticles:  The Influence of Size, Shape, and Dielectric Environment

Dust Extinction Curves and Lyα Forest Flux Deficits for Use in Modeling Gamma‐Ray Burst Afterglows and All Other Extragalactic Point Sources

DFT investigation of the adsorption of atomic hydrogen on a cluster-model graphite surface

MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS

The Spectral Results of the Far‐Infrared Absolute Spectrophotometer Instrument onCOBE

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

A 3% SOLUTION: DETERMINATION OF THE HUBBLE CONSTANT WITH THEHUBBLE SPACE TELESCOPEAND WIDE FIELD CAMERA 3

GC-IRS13E—A PUZZLING ASSOCIATION OF THREE EARLY-TYPE STARS

THE STAR FORMATION HISTORY OF THE MILKY WAY'S NUCLEAR STAR CLUSTER

Improved Distances to Type Ia Supernovae with Multicolor Light‐Curve Shapes: MLCS2k2

Spatially Resolved Millimeter Interferometry of SMM J02399−0136: AVery Massive Galaxy atz= 2.8

Carbon Onions as Possible Carriers of the 2175 A Interstellar Absorption Bump

Dust extinction and absorption: the challenge of porous grains

Carbon in the Universe

Infrared Extinction toward Nearby Star‐forming Regions

The VIIth catalogue of galactic Wolf–Rayet stars

Interstellar Dust Models Consistent with Extinction, Emission, and Abundance Constraints

The history of star formation in dusty galaxies

Influence of the angular response on Fourier absolute spectrometry the case of COBE-FIRAS

TheCOBEDiffuse Infrared Background Experiment Search for the Cosmic Infrared Background. IV. Cosmological Implications

The Spectrum of the Extragalactic Far‐Infrared Background from theCOBEFIRAS Observations

SPATIALLY RESOLVING THE HK Tau B EDGE-ON DISK FROM 1.2 TO 4.7 μm: A UNIQUE SCATTERED LIGHT DISK

SN 2006gy: Discovery of the Most Luminous Supernova Ever Recorded, Powered by the Death of an Extremely Massive Star like η Carinae

Quantitative studies of the optical and UV spectra of Galactic early B supergiants

The intrinsic ultraviolet continua of O stars

An analysis on the shapes of ultraviolet extinction curves. I - The 2175 A bump

Interstellar extinction in the infrared - The molecular cloud toward HD 62542

Fundamental Properties and Distances of the Large Magellanic Cloud from Eclipsing Binaries. II. HV 982

Calibration of the COBE FIRAS instrument

The Discordance of Mass‐Loss Estimates for Galactic O‐Type Stars

Ultraviolet observations of interstellar extinction near the Cepheus OB3 molecular cloud

Peculiar ultraviolet interstellar extinction

An analysis of the shapes of ultraviolet extinction curves. II - The far-UV extinction

The [ITAL]IUE[/ITAL] MEGA Campaign: Modulated Structure in the Wind of HD 64760 (B0.5 Ib)

Determining the Physical Properties of the B Stars. I. Methodology and First Results

AN ANALYSIS OF THE SHAPES OF INTERSTELLAR EXTINCTION CURVES. VI. THE NEAR-IR EXTINCTION LAW

An analysis of the shapes of ultraviolet extinction curves. III - an atlas of ultraviolet extinction curves

Wind Variability of B Supergiants. I. The Rapid Rotator HD 64760 (B0.5 Ib)

Ultraviolet extinction toward five open clusters, and the accuracy of IUE extinction measurements

[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Spectroscopy of the O [CSC]vi[/CSC] Resonance Doublet in Sand 2 (WO)

A catalog of ultraviolet interstellar extinction excesses for 1415 stars

The [ITAL]IUE[/ITAL] MEGA Campaign: The Rotationally Modulated Wind of ζ Puppis

The variability of UV extinction-curve shapes and its impact upon dereddened UV energy distributions