By means of a modified thermophysical model (TPM) that takes into account asteroid shape and pole uncertainties, we analyze the thermal infrared data acquired by the NASA's Wide-field Infrared Survey Explorer (WISE) of about 300 asteroids with derived convex shape models. We adopt convex shape models from the DAMIT database (Durech et al., 2010, A
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Thermal Intertias of Main-Belt Asteroids from Wise Thermal Infrared DataHanus, J. et al.112014
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Thermodynamic fluctuations in solar photospheric three-dimensional convection simulations and observations
Not Available
Beck, C. et al.Fecha de publicación:
112013 -
Thick Disks of Edge-on Galaxies Seen through the Spitzer Survey of Stellar Structure in Galaxies (S4G): Lair of Missing Baryons?
Most, if not all, disk galaxies have a thin (classical) disk and a thick disk. In most models thick disks are thought to be a necessary consequence of the disk formation and/or evolution of the galaxy. We present the results of a study of the thick disk properties in a sample of carefully selected edge-on galaxies with types ranging from T = 3 to T
Comerón, Sébastien et al.Fecha de publicación:
112011 -
Thin shell formation in radiative shocks. 1: Supernova remnants in low-density media
This paper explores the onset of thin-shell formation in interstellar shocks associated with supernova explosions. We outline a simple but useful scheme that indicates the time at which thin shell formation begins for supernova remnants (SNRs) evolving in a range of interstellar environments, extending the previous analytical models to arbitrary
Tenorio-Tagle, G. et al.Fecha de publicación:
111994 -
Thinking Hattusha: Astronomy and Landscape in the Hittite Lands
Not Available
González-García, A. C. et al.Fecha de publicación:
112011 -
Three dimensional structure of a regular sunspot from the inversion of IR Stokes profiles
The magnetic, thermal and velocity structure of a regular sunspot, observed close to solar disk center is presented. Spectropolarimetric data obtained with the Tenerife Infrared Polarimeter (TIP) in two infrared FeI lines at 15 648.5 Å and 15 652.8 Å are inverted employing a technique based on response functions to retrieve the atmospheric
Mathew, S. K. et al.Fecha de publicación:
112003