[PDF] Top 20 Linking simple molecules to grain evolution across planet-forming disks
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Linking simple molecules to grain evolution across planet-forming disks
... of simple deuterated molecules in comparison to their non-deuterated ...protoplanetary disks, where deuterium enrichment takes place, the ionization source comes from galac- tic cosmic rays (CRs) and ... See full document
143
Gas and dust chemistry in planet forming disks
... the planet-forming ...the evolution of material in young stellar objects (YSOs) are thus essential for addressing these ...prebiotic molecules and planets that can sustain ...“debris” ... See full document
12
Water in Planet Forming Disks
... complex molecules such as polycyclic aromatic hydrocarbons ...protoplanetary disks have been developed by a number of research groups (see Table 3), taking into account the wide range of radiation fi elds ... See full document
24
Detection and Characterization of Extrasolar Planets through Planet-Disk Dynamical Interactions
... the planet that can open a detectable gap depends on the re- solving capabilities of the observational facility taking the ...(i.e., disks with observed azimuthally asymmetric MMR gaps) that has yet been ... See full document
171
Evolution of HLA Class II Molecules: Allelic and Amino Acid Site Variability Across Populations
... from empirically derived mutation rates and population Despite difficulties with independence of genetic in- sizes is difficult, given the uncertainty in estimates of formation, there exists strong evidence of balanced ... See full document
8
Brown Dwarf Disks with ALMA
... these disks. This result confirms the recent finding that the evolution of solids up to these sizes proceeds in a similar way in disks around brown dwarfs/very low mass stars as in disks ... See full document
15
The Depletion of Water During Dispersal of Planet-forming Disk Regions
... most disks as coming from an optically thick surface layer within the snow line radius, at temperatures of 300 – 700 K ( Carr & Najita 2011; Salyk et ...in disks ( ...four disks with VLT-VISIR ... See full document
23
A Multi-wavelength Analysis of Dust and Gas in the SR 24S Transition Disk
... the disks in scattered light seem to be extended enough to fi ll the effective Roche radius of the system, probing tidal interactions between the two disks ( Mayama et ... See full document
11
Sequential planet formation in the HD 100546 protoplanetary disk?
... maximum grain size that particles can reach under these as- ...maximum grain size is one order of magnitude lower than the size corresponding to S t = 1, which are the parti- cles that feel the highest ... See full document
12
Dust Polarization toward Embedded Protostars in Ophiuchus with ALMA. I. VLA 1623
... Magnetic fields are expected to impact the forma- tion of protostars and their disks. Theoretical stud- ies show that angular momentum of infalling mate- rial is transported outward by magnetic fields. This ... See full document
15
Fundamental Molecules and Mechanisms for Forming and Maintaining Neuromuscular Synapses
... Although it had long been appreciated that motor neuron-derived factors played an important role in postsynaptic differentiation, including clustering of AChRs, the critical neuronal factors remained undiscovered through ... See full document
19
The first steps of planet formation : studying grain growth with millimetre interferometers
... of grain growth has become much clearer over the last few years, several quanti- tative details are still under ...which grain growth occurs and how this relates to the disc’s physi- cal structure ... See full document
158
The accumulation and trapping of grains at planet gaps : effects of grain growth and fragmentation
... that planet gaps were more easily opened in the dust phase than in the ...increasing planet mass and varied with grain ...massive planet, on horseshoe ...grains across a large size ... See full document
14
GA40 0100 PLAN 4000 General Information Manual Nov82 pdf
... Network interface cards are similar to controller cards, linking workstations to the file servers and their shared hard disks in the same way that controller cards link microcomputers to[r] ... See full document
35
Diaquabis(μ 4 hydroxybenzenecarboxylato κ2O,O′)disilver(I)(Ag—Ag) tetrahydrate
... ORTEP-3 (Farrugia, 1997) drawing of (I) with the atomic numbering scheme. Displacement ellipsoids are drawn at the 50% probability level. Hydrogen bonds are shown as dashed lines. Unlabelled atoms are related to labelled ... See full document
7
Linking Entities Across Images and Text
... The extraction of relations across text and image is a new area for research. We showed in this pa- per that we could use semantic and statistical func- tions to link the entities in an image to mentions of the ... See full document
9
Orbital evolution of a circumbinary planet in a gaseous disk
... a planet formed in the outer region in a protoplanetary disk migrates into the unstable ...the planet halts at the disk’s inner ...the planet expe- riences a severe gravitational perturbation in the ... See full document
12
2 (4 Bromophenyl) N (pyrazin 2 yl)acetamide
... In (I) the dihedral angle between the mean planes of the 4-Bromophenyl and pyrazine rings is 54.6 (3)° (Fig. 1). An intramolecular C—H···O hydrogen bond generates an S(6) graph-set motif. Bond lengths are in normal ... See full document
7
The JCMT Gould Belt Survey: Evidence for Dust Grain Evolution in Perseus Star-forming Clumps
... example of this behavior. Interestingly, many low β re- gions also coincide with the locations of bipolar outflows, prompting us to suspect that outflows may be capable of carrying lower β grains from deep within a ... See full document
25
Molecular Spectroscopy of Planet-Forming Regions in Circumstellar Disks
... the disks of gas and dust that form around collapsing protostars as a consequence of angular momentum ...Circumstellar disks and planetary systems are both well-studied, and the set of processes that ... See full document
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