Lee Hartmann
0000-0003-1430-8519
University of Michigan
163 papers found
Refreshing results…
Gravitational Focusing and the Star Cluster Initial Mass Function
Radio Measurements of the Stellar Proper Motions in the Core of the Orion Nebula Cluster
The Gould’s Belt Distances Survey (Gobelins). Iii. The Distance to the Serpens/Aquila Molecular Complex
The Gould’s Belt Distances Survey (Gobelins). I. Trigonometric Parallax Distances and Depth of the Ophiuchus Complex
The Gould’s Belt Distances Survey (Gobelins). Ii. Distances and Structure Toward the Orion Molecular Clouds
Illuminating the Role of Spiral Waves in Circumstellar Disks
The Spiral Wave Instability Induced by a Giant Planet. I. Particle Stirring in the Inner Regions of Protoplanetary Disks
Accretion onto Pre-Main-Sequence Stars
Self-Destructing Spiral Waves: Global Simulations of a Spiral-Wave Instability in Accretion Disks
VizieR Online Data Catalog: Spectroscopic binary population of ONC and NGC2264 (Kounkel+, 2016)
VizieR Online Data Catalog: The Herschel Orion Protostar Survey (HOPS): SEDs (Furlan+, 2016)
VizieR Online Data Catalog: NIR survey of Spitzer YSOs in Orion Mol. Cloud (Kounkel+, 2016)
The Herschel Orion Protostar Survey: Spectral Energy Distributions and Fits Using a Grid of Protostellar Models
ANHSTSURVEY FOR 100–1000 Au COMPANIONS AROUND YOUNG STELLAR OBJECTS IN THE ORION MOLECULAR CLOUDS: EVIDENCE FOR ENVIRONMENTALLY DEPENDENT MULTIPLICITY
Spectroscopic Binaries in the Orion Nebula Cluster and NGC 2264
Planetary Signatures in the Sao 206462 (Hd 135344b) Disk: A Spiral Arm Passing Through Vortex?
VizieR Online Data Catalog: Spitzer observations of Taurus members (Luhman+, 2010)
Csi 2264: Characterizing Young Stars in Ngc 2264 With Stochastically Varying Light Curves
CSI 2264: SIMULTANEOUS OPTICAL AND INFRARED LIGHT CURVES OF YOUNG DISK-BEARING STARS IN NGC 2264 WITHCoRoTandSPITZER—EVIDENCE FOR MULTIPLE ORIGINS OF VARIABILITY
Thespitzerspace Telescopesurvey of the Orion a and B Molecular Clouds. I. A Census of Dusty Young Stellar Objects and a Study of Their Mid-Infrared Variability
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