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Nuria Calvet
Researcher at University of Michigan
Publications - 243
Citations - 27758
Nuria Calvet 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 85, co-authored 234 publications receiving 26474 citations. Previous affiliations of Nuria Calvet include Centro de Investigaciones de Astronomia & Harvard University.
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Accretion and the Evolution of T Tauri Disks
TL;DR: Gullbring et al. as discussed by the authors estimate disk accretion rates for pre-main-sequence stars in the Taurus and Chamaeleon I molecular cloud complexes using a minimum of parameters.
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Intrinsic near-infrared excesses of T tauri stars: Understanding the classical T tauri star locus
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Disk accretion rates for T tauri stars
Erik Gullbring,Lee Hartmann,Cesar Briceno,Cesar Briceno,Cesar Briceno,Nuria Calvet,Nuria Calvet +6 more
TL;DR: In this paper, the authors present new measurements of disk accretion rates for T Tauri stars in the Taurus molecular cloud complex, which are based on intermediate-resolution spectrophotometry from 3200 to 5200 A, and derive the excess hot continuum emission produced by accretion onto the central star.
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The Structure and Emission of the Accretion Shock in T Tauri Stars
TL;DR: In this article, the structure and spectral energy distribution of the emergent continuum emission from a shock at the base of the magnetospheric accretion column were analyzed for T Tauri stars, and it was shown that the spectral shape of the excess can be understood as optically thick emission from the heated photosphere below the shock, appearing mostly on the Paschen and Brackett continua, and optically thin emission from preshock and attenuated postshock regions, dominating at wavelengths shorter than the Balmer threshold.
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Accretion Disks around Young Objects. I. The Detailed Vertical Structure
TL;DR: In this article, the authors discussed the properties of an accretion disk around a star with parameters typical of T T Tauri stars and with the average accretion rate for these disks.