L
Lee Hartmann
Researcher at University of Michigan
Publications - 590
Citations - 60559
Lee Hartmann is an academic researcher from University of Michigan. The author has contributed to research in topics: Stars & T Tauri star. The author has an hindex of 134, co-authored 579 publications receiving 57649 citations. Previous affiliations of Lee Hartmann include University of Hawaii & National Science Foundation.
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Journal Article
Ultraviolet Observations of Metal Deficient Field Giants
Journal ArticleDOI
The missing cavities in the SEEDS polarized scattered light images of transitional protoplanetary disks: a generic disk model
Ruobing Dong,Roman R. Rafikov,Zhaohuan Zhu,Lee Hartmann,Barbara A. Whitney,Timothy D. Brandt,Takayuki Muto,Takayuki Muto,Jun Hashimoto,Carol A. Grady,Katherine B. Follette,Masayuki Kuzuhara,Ryoko Tanii,Yoichi Itoh,Christian Thalmann,John P. Wisniewski,Satoshi Mayama,Markus Janson,Lyu Abe,Wolfgang Brandner,Joseph C. Carson,Sebastian Egner,Markus Feldt,Miwa Goto,Olivier Guyon,Yutaka Hayano,Masahiko Hayashi,Saeko S. Hayashi,Thomas Henning,Klaus W. Hodapp,Mitsuhiko Honda,Shu-ichiro Inutsuka,Miki Ishii,Masanori Iye,Ryo Kandori,G. R. Knapp,Tomoyuki Kudo,Nobuhiko Kusakabe,Taro Matsuo,Michael W. McElwain,Shoken Miyama,Jun-Ichi Morino,Amaya Moro-Martin,Tetsuro Nishimura,Tae-Soo Pyo,Hiroshi Suto,Ryuji Suzuki,Michihiro Takami,Naruhisa Takato,Hiroshi Terada,Daigo Tomono,Edwin L. Turner,Edwin L. Turner,Makoto Watanabe,Toru Yamada,Hideki Takami,Tomonori Usuda,Motohide Tamura +57 more
TL;DR: In this article, a generic disk model that can simultaneously account for the general features in IRS, SMA, and Subaru observations is presented, and the scattered light images for this model are computed, which agree with the general trend seen in Subaru data.
Posted Content
Star Formation: Lessons from Taurus
TL;DR: The Taurus molecular cloud complex is the paradigm for quiescent, low-density, isolated star formation as discussed by the authors, and the age distribution of its stellar population indicates that star formation is a rapid and dynamic process, inconsistent with the old picture of magnetically controlled protostellar cloud collapse.
Posted Content
Evolution of Disk Accretion
TL;DR: In this paper, the authors review the present knowledge of disk accretion in young low mass stars, and in particular, the mass accretion rate and its evolution with time, and they suggest that the low-mass accretion rates of the latter objects require episodes of high mass accuration rate to build the bulk of the star.
Journal ArticleDOI
The Gould's Belt Very Large Array Survey I: The Ophiuchus complex
Sergio A. Dzib,Laurent Loinard,Laurent Loinard,Amy J. Mioduszewski,Luis F. Rodríguez,Luis F. Rodríguez,Gisela N. Ortiz-León,Gerardo Pech,Juana L. Rivera,Rosa M. Torres,Andrew F. Boden,Lee Hartmann,Neal J. Evans,Cesar Briceno,John J. Tobin +14 more
TL;DR: In this paper, the authors presented large-scale radio observations of the Ophiuchus star-forming complex obtained with the Karl G.\ Jansky Very Large Array at 4 and 6 cm.