Results 51 to 60 of about 9,757 (190)

Inside-Out Evacuation of Transitional Protoplanetary Disks by the Magneto-Rotational Instability

, 2007
How do T Tauri disks accrete? The magneto-rotational instability (MRI) supplies one means, but protoplanetary disk gas is typically too poorly ionized to be magnetically active. Here we show that the MRI can, in fact, explain observed accretion rates for
AE Glassgold, AE Glassgold, B König, BT Draine, C Salyk, CF Gammie, E Bergin, Eugene Chiang, J Igea, J Muzerolle, JA Eisner, JF Hawley, JH Kastner, JR Najita, K Strom, L Hartmann, M Güdel, M Oppenheimer, MW Kunz, N Calvet, N Calvet, OM Blaes, P D’Alessio, P Goldreich, RD Alexander, Ruth Murray-Clay, S Fromang, S Matsumura, SA Balbus, SJ Weidenschilling, SJ Wolk, T Umebayashi, TP Fleming   +32 more
core   +2 more sources

The libreas in Ferdinand the Catholic Entourage: Relationships and Representations of the Cortesan Powers

Studia Historica. Historia Medieval, 2018
This paper reflects about the political use of liveries in Ferdinand the Catholic’s Court. The aim of this study is to better understand dress-given in the royal court and its political implications in the court society.
Germán GAMERO IGEA
doaj   +1 more source

Accretion Outbursts in Circumplanetary Disks

, 2012
We describe a model for the long term evolution of a circumplanetary disk that is fed mass from a circumstellar disk and contains regions of low turbulence (dead zones).
Lubow, S. H., Martin, R. G.
core   +1 more source

Design of a Sensor-Based Digital Product Passport for Low-Tech Manufacturing: Traceability and Environmental Monitoring in Bio-Block Production

Sensors
The Digital Product Passport (DPP) is an emergent strategic tool poised to significantly enhance traceability, circularity, and sustainability within industrial supply chains, aligning with evolving European Union regulatory frameworks.
Alessandro Pracucci, Matteo Giovanardi
doaj   +1 more source

A New Probe of the Planet-Forming Region in T Tauri Disks

, 2004
We present new observations of the FUV (1100-2200 Angstrom) radiation field and the near- to mid-IR (3--13.5 micron) spectral energy distribution (SED) of a sample of T Tauri stars selected on the basis of bright molecular disks (GM Aur, DM Tau, LkCa15).
Abgrall H., Chunhua Qi, David K. Lynch, Dutrey A., D’Alessio P., Edwin Bergin, Evelyne Roueff, Gregory J. Herczeg, Herve Abgrall, Michael L. Sitko, Nuria Calvet, Paola D'Alessio, R. Brad Perry, Ray W. Russell, Suellen M. Brafford   +14 more
core   +2 more sources

High-resolution Spectroscopy of [Ne II] Emission from TW Hya [PDF]

, 2007
We present high-resolution echelle spectra of [Ne II] 12.81 micron emission from the classical T Tauri star (CTTS) TW Hya obtained with MICHELLE on Gemini North.
Bohm T., Gregory J. Herczeg, Ilaria Pascucci, Joan R. Najita, Lynne A. Hillenbrand   +4 more
core   +1 more source

Povezava evidenc s področja graditve in katastra nepremičnin ( = Integration of Records in the Field of Building Construction and Real Estate Cadastre)

Geodetski Vestnik
This paper presents the introduction of the building plot as a new entity in the Real Estate Cadastre, established on the basis of data from the eConstruction (eGraditev) system.
Rok Cedilnik, Miha Muck, Marijana Vugrin
doaj   +1 more source

Antibody-drug conjugates in treating older patients suffering from cancer: what is the real value?

Human Vaccines & Immunotherapeutics, 2021
Immunotherapeutic drugs and target therapies have represented an epochal change in treating cancer patients. They represent an attractive option in oncologists’ armamentarium, particularly if we consider the optimal balance between efficacy and toxicity.
Gianluca Perego, Antonio Ghidini, Andrea Luciani, Fausto Petrelli   +3 more
doaj   +1 more source

Arquero Caballero, Guillermo F.: "El confesor real en la Castilla de los Trastámara 1366-1504".

Los Libros de la Corte.es, 2023
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Germán Gamero Igea
doaj  

Meridional circulation of gas into gaps opened by giant planets in three-dimensional low-viscosity disks

, 2014
We examine the gas circulation near a gap opened by a giant planet in a protoplanetary disk. We show with high resolution 3D simulations that the gas flows into the gap at high altitude over the mid-plane, at a rate dependent on viscosity.
Bitsch, B., Crida, A., Kanagawa, K., Lega, E., Morbidelli, A., Szulagyi, J., Tanigawa, T.   +6 more
core   +2 more sources