[PDF] Top 20 High angular resolution studies of protoplanetary discs
Has 10000 "High angular resolution studies of protoplanetary discs" found on our website. Below are the top 20 most common "High angular resolution studies of protoplanetary discs".
High angular resolution studies of protoplanetary discs
... The physical processes that shape circumstellar discs during their evolution ultimately determine the amount of material available for, and the timescale of the planet for- mation. The dust grain growth and ... See full document
166
High Angular Resolution Diffusion Imaging Probabilistic Tractography of the Auditory Radiation
... vestigate the microstructure of the auditory radiation in these neuropsychiatric disorders. The findings in our study indicate that more detailed and robust measures of the auditory radiation can be obtained by HARDI ... See full document
6
Revealing signatures of planets migrating in protoplanetary discs with ALMA multiwavelength observations
... obtaining high resolution data becomes more challenging due to the exceptional weather conditions ...both high spa- tial resolution and high sensitivity would be required to see the ... See full document
12
Imaging polarimetry for the characterisation of exoplanets and protoplanetary discs : scientific and technical challenges
... a high school degree in science I obtained a bachelor’s degree in Aerospace Engineering at the Technical University of Madrid, in ...these studies I obtained a Rafael Calvo Rodes fellowship to work for two ... See full document
187
Lights and shadows : multi wavelength analysis of young stellar objects and their protoplanetary discs
... In order to find possible patterns in the luminosity changes, the analysis of variability requires observations over at least several days to detect Type I variations, based on Herbst et al. (1994) classification, but ... See full document
257
High resolution Millimeter Imaging of the CI Tau protoplanetary disk : a massive ensemble of protoplanets from 0 1 to 100 au
... High-resolution ALMA studies are steadily increasing the census of disks with annular substructure. Although unique in being the only such system with a hot Jupiter, CI Tau ’ s ring structure is not ... See full document
7
Accretion discs as regulators of stellar angular momentum evolution in the ONC and Taurus Auriga
... early studies of PMS AM evolution in the ONC relied on NIR excesses and H α equivalent widths (EW) to ascer- tain whether a PMS star hosted a circumstellar disc or was actively accreting, ...of discs ... See full document
20
Physics of cosmic plasmas from high angular resolution X-ray imaging of galaxy clusters
... by high-resolution X-ray imaging of galaxy ...such studies. In this white paper, we discuss why we need arcsecond-resolution, high collecting area, low relative background X-ray imagers ... See full document
9
Using high angular resolution diffusion imaging data to discriminate cortical regions
... very high levels of cytochrome oxidase it may be expected that it is easily ...higher resolution DWI data: at higher resolution several samples could be taken from different depths to increase the ... See full document
10
Development of High Angular Resolution Diffusion Imaging Analysis Paradigms for the Investigation of Neuropathology
... research studies investigating neuronal development [72], as well as specific diseases such as attention deficit hyperactivity disorder [94] and schizophrenia ... See full document
141
The pti carbon star angular size survey: effective temperatures and non-sphericity
... Recent studies have shown that certain stars can take on a non-spherical appearance due to the effects of surface inho- mogeneities (Chiavassa et ...very high resolution but not particularly well ... See full document
19
The relationship between Class I and Class II methanol masers at high angular resolution
... achieved high detection rates (Chen et ...our high-resolution data allow us to directly confirm the presence of class I maser components within these outflow ... See full document
18
MOA 2016 BLG 227Lb: a massive planet characterized by combining light curve analysis and Keck AO imaging
... With this method, it might seem that no assumptions are required regarding the probability of the microlens stars hosting planets, and there would be no biases due to any inadequacies of the Galactic model used. However, ... See full document
15
PubMedCentral-PMC5152949.pdf
... High angular resolution diffusion imaging (HARDI) has recently been of great interest in mapping the orientation of intra-voxel crossing fibers, and such orientation information allows one to infer ... See full document
22
The JCMT Gould Belt Survey : low mass protoplanetary discs from a SCUBA 2 census of NGC 1333
... substantial discs than the remnants around Class III weak-line sources, without the confusion of circumstellar envelopes that dominate in Class I/0 protostellar ... See full document
6
Temporal Evolution of Disc in Young Patients with Low Back Pain and Stress Reaction in Lumbar Vertebrae
... bral discs (L4 –5 and L5–S1; also shown in magnified images) around the stressed segment demonstrated the presence of annular fissures (arrows), disc herniation, and nuclear degen- eration at ... See full document
6
High-resolution spatiotemporal weather models for climate studies
... temporal resolution, and temporal coverage of these measurements are high, the observations are made at specific geographic points which do not represent the entire ...Previous studies of the ... See full document
8
High resolution electron microscope studies of chromosomal fibers
... High resolution-high contrast sensitive films directly exposed by the electron beam are at present the best method of transferring information from the beam to a photographic image... In[r] ... See full document
128
Structural variety in ytterbium dicarboxylate frameworks and in situ study diffraction of their solvothermal crystallisation
... Nitrogen adsorption isotherms of ( 1 ) and ( 2 ) were recorded at 77 K after degassing under a vacuum at chosen temperature (see below) using a Micromeritics ASAP 2010 ap- paratus. Surface areas were calculated using the ... See full document
11
NOEMA complementarity with NIKA2
... core compared to those with many low-mass cores may be explained by different formation mechanisms that coexist, or even interplay, or by di ff erences in the initial density profiles and / or magnetic field properties ... See full document
6
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