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.
Papers
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Journal ArticleDOI
Protostars in the Elephant Trunk Nebula
William T. Reach,Jeonghee Rho,Erick T. Young,James Muzerolle,Sergio Fajardo-Acosta,Lee Hartmann,Aurora Sicilia-Aguilar,Lori Allen,Sean Carey,Jean-Charles Cuillandre,Thomas H. Jarrett,Patrick Lowrance,A. P. Marston,Alberto Noriega-Crespo,Robert L. Hurt +14 more
TL;DR: The optically dark globule IC 1396A is revealed using Spitzer Space Telescope images at 3.6, 4.5, 5.8, 8, and 24 μm to be infrared-bright and to contain a set of previously unknown protostars.
Journal ArticleDOI
The Herschel Orion Protostar Survey: Luminosity and Envelope Evolution
William J. Fischer,William J. Fischer,S. Thomas Megeath,Elise Furlan,Babar Ali,Amelia M. Stutz,Amelia M. Stutz,John J. Tobin,John J. Tobin,Mayra Osorio,Thomas Stanke,P. Manoj,Charles A. Poteet,Joseph Booker,Lee Hartmann,T. L. Wilson,Philip C. Myers,Dan M. Watson +17 more
TL;DR: In this paper, the bolometric luminosities and temperatures for 330 Orion YSOs, 315 of which have bolometric temperatures characteristic of protostars, were analyzed using fits to the spectral energy distributions (SEDs).
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Identifying Primordial Substructure in NGC 2264
Paula S. Teixeira,Paula S. Teixeira,Charles J. Lada,Erick T. Young,Massimo Marengo,August Muench,James Muzerolle,Nick Siegler,George H. Rieke,Lee Hartmann,S. Thomas Megeath,Giovanni G. Fazio +11 more
TL;DR: In this article, the Spitzer Space Telescope observations of the young cluster NGC2264 have been used to identify the most highly embedded and youngest objects in the cluster, and the majority of these sources are found to be protostellar in nature with Class I spectral energy distributions.
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Detection of Disk Accretion at the Substellar Limit
James Muzerolle,James Muzerolle,James Muzerolle,Cesar Briceno,Cesar Briceno,Nuria Calvet,Nuria Calvet,Lee Hartmann,Lynne A. Hillenbrand,Erik Gullbring +9 more
TL;DR: The first definitive detection of disk accretion in an object near or below the substellar limit was made in this paper, where the authors obtained an echelle-resolution spectrum of the very low mass T Tauri star V410 Anon 13; the emission-line profile of Hα clearly exhibits the large line width and asymmetry characteristic of a freefalling accretion flow.
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A proper motion survey for pre-main-sequence stars in Taurus-Auriga
TL;DR: In this paper, a proper motion survey of pre-main-sequence stars near the Taurus-Auriga molecular cloud is presented, with 209 possible Taurus proper motion members selected from an initial sample of 4600 stars with V ≥ 16 in a 8.9 square degree region.