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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WWW Database of Models of Accretion Disks Irradiated by The Central Star
TL;DR: In this paper, a catalog of physical models of irradiated accretion disks around young stars based on the modelling techniques by D'Alessio et al. is presented, which includes disk models for different central stars, disk sizes, inclinations, dust contents and mass accretion rates.
Peer Review
An ACA 870 μ m Continuum Survey of Orion Protostars and their Evolution
S. R. Federman,S. T. Megeath,John J. Tobin,Patrick D. Sheehan,Riwaj Pokhrel,Nolan M. Habel,Amelia M. Stutz,William J. Fischer,Lee Hartmann,Thomas Stanke,Mayank Narang,Mayra Osorio,Prabhani Atnagulov,R. Rahatgaonkar +13 more
TL;DR: In this article , the Atacama Compact Array (ACA) was used to measure protostellar flux densities on envelope scales ≤ 8000 AU (20) and resolve the structure of envelopes with 1600 AU (4) resolution.
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Extension of HOPS out to 500 pc (eHOPS). I. Identification and Modeling of Protostars in the Aquila Molecular Clouds
Riwaj Pokhrel,S. T. Megeath,Robert A. Gutermuth,Elise Furlan,William J. Fischer,S. R. Federman,John J. Tobin,Amelia M. Stutz,Lee Hartmann,Mayra Osorio,Dan M. Watson,Thomas Stanke,P. Manoj,Mayank Narang,Prabhani Atnagulov,Nolan M. Habel,Wafa Zakri +16 more
TL;DR: In this paper , a Spitzer/Herschel focused survey of the Aquila molecular clouds (d ∼ 436 pc) is presented as part of the eHOPS (extension of the Herschel orion protostar survey, or HOPS, Out to 500 ParSecs) census of nearby protostars.
Theoretical studies of the outer envelopes of young stellar objects
TL;DR: In this paper, a grid was computed of models of scattering in a disk+envelope system, and it was shown that the wind of the pre-main sequence object FU Orionis arises from the surface of the luminous prostellar accretion disk.
Journal ArticleDOI
Probing the Protostellar Envelope around L1157: the Dust and Gas Connection
TL;DR: In this article, the authors present observations of the Class 0 protostar L1157-mm using the Combined Array for Research in Millimeter-wave Astronomy (CARMA) in 3 mm dust continuum and N2H+ line emission.