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Nonparametric Bayesian Learning for Collaborative Robot Multimodal Introspection
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CIA Reading Room cia-rdp84-00581r000401320059-4: EAST EUROPEAN & UP FR: PFANZENSRT TO: PHYS STAT SOL
illo bliport-anco of Appliod !--ntomology for i-lantirotertlon, by iL. P..waGEP;AN, per, Der Pfla;~ d, No 9. 1967. pp 100-103.ACZ I J-4241,~ID 220400:2~68tici--b and'",May 68356.163. hytolAthological ...
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The Official Raspberry Pi Handbook 2023
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Fundamental Astronomy
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Intercultural Dialogue in the European Education Policies
A Conceptual Approach...
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CIA Reading Room cia-rdp91-00772r000301590035-2: A FR: PADIATRIE TO: PERVYY VSESCYUZNYY SIMPOZIUM.
iot; un tic rir Wro (j4~ i ~., I Al orsOriglooli Articli C K*ckod,!; I e 11' 1., 4:1 : IJ tec:jl- !, ;,,: ~i I i, rt I't I;er t*J ~-o- j". '.4!~' fKAM)i - I (.' J ~t I t I , - t; !. i .. t;I,m fll~ e ...
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Planet formation signposts: observability of circumplanetary disks via gas kinematics
The identification of on-going planet formation requires the finest angular resolutions and deepest sensitivities in observations inspired by state-of-the-art numerical simulations. Hydrodynamic simul...
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DTIC ADA609742: Separated Fringe Packet Observations with the CHARA Array. II. Omega Andromeda, HD 1
When observed with optical long-baseline interferometers, components of a binary star that are sufficiently separated produce their own interferometric fringe packets; these are referred to as separat...
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Cassini States with Dissipation: Why Obliquity Tides Cannot Inflate Hot Jupiters
Some short-period exoplanets (hot Jupiters) are observed by their transits to have anomalously large radii. It has been suggested that these planets are in a resonance involving persistent misalignmen...
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The Matryoshka Disk: Keck/NIRC2 Discovery of a Solar System-Scale, Radially Segregated Residual Prot
Using Keck/NIRC2 $L^\prime$ (3.78 $\mu m$) data, we report the direct imaging discovery of a scattered light-resolved, solar system-scale residual protoplanetary disk around the young A-type star HD 1...
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Star Formation in Relic HII Regions of the First Stars: Binarity and Outflow Driving
Star formation in relic HII regions of the first stars is investigated using magneto-hydrodynamical simulations with a nested grid method that covers 10 orders of magnitude in spatial scale and 20 ord...
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Introduction to Logic Circuits & Logic Design with Verilog
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What next for the Likely Pre-Supernova, HD 179821?
We have used the Owens Valley Radio Observatory Millimeter Array to obtain a map of the J = (1-0) CO emission from the circumstellar shell around HD 179821, a highly evolved G-type star which will pro...
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Diamonds in HD 97048
We present adaptive optics high angular resolution ($\sim0\farcs$1) spectroscopic observations in the 3 $\mu$m region of the Herbig Ae/Be star HD 97048. For the first time, we spatially resolve the em...
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Evolution of the Planetary Obliquity: The Eccentric Kozai-Lidov Mechanism Coupled with Tide
Evolution of the Planetary Obliquity: The Eccentric Kozai-Lidov Mechanism Coupled with Tide 作者： Xiumin Huang 1,2 Jianghui Ji 1,2,3 Shangfei Liu 4 Ruobing Dong 5 Su Wang 1,3 作者单位： 1. CA...
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Retro Gaming with Raspberry Pi
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The diameter of the CoRoT target HD 49933. Combining the 3D limb darkening, asteroseismology, and in
Context. The interpretation of stellar pulsations in terms of internal structure depends on the knowledge of the fundamental stellar parameters. Long-base interferometers permit us to determine very a...
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Optics in Our Time
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High Density Lipoproteins
From Biological Understanding to Clinical Exploitation...
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Introduction to Logic Circuits & Logic Design with VHDL
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WR 110: A Single Wolf-Rayet Star With Corotating Interaction Regions In Its Wind?
A 30-day contiguous photometric run with the MOST satellite on the WN5-6b star WR 110 (HD 165688) reveals a fundamental periodicity of P = 4.08 +/- 0.55 days along with a number of harmonics at period...
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Resolved Submillimeter Observations of the HR 8799 and HD 107146 Debris Disks
We present 880 um Submillimeter Array observations of the debris disks around the young solar analogue HD 107146 and the multiple-planet host star HR 8799, at an angular resolution of 3" and 6", respe...
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The First Jet in the Universe: Protostellar Jets from the First Stars
The protostellar jets driven by the formation of the first stars are studied by using MHD nested grid simulations. Starting from a slowly rotating spherical cloud of 5.1 times 10^4 Msun permeated by a...
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CIA Reading Room cia-rdp84-00581r000200740030-2: AUTHORS FR: POMBIA, F. TO: PONOMARENKO, I.I.
IfCLU~zttttj,, bir I. Pmelav,, 12'MSIMf., per,, Kmmmistp Na 33 MaY I~K>U.,PP T 58-6' Ir 0.JPItS 367ligUSOFolscipt 66 303,3S)ilwav 1. 9 Poe20 A-19 196.1,-. Pp- 3-4-/D vummPOXOct. 66ft'.)ICUe, 3a tbi...
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Wetlands and Water Framework Directive
Protection, Management and Climate Change...
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CIA Reading Room cia-rdp74-00005r000200030001-9: HANDBOOK FOR SUBJECT FILING RECORDS MAINTENANCE REC
l pproved For Rel a 1~ / 9 ~,,_v P74-08005R0002~0030001-9 6 A~ 1959 HANDBOOK FOR SUBJECT FILING S MAINTENANCE RECORDS MANAGEMENT PROGRAM i4p~?oved For ReFease--499~/09f07-:- CIAt-RDP74-00{}05ft00?-2~A...
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Dissonant Heritages and Memories in Contemporary Europe
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The Official Raspberry Pi Handbook 2022
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Problems in Classical Electromagnetism
157 Exercises with Solutions...
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Interferometry and Synthesis in Radio Astronomy
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Raspberry Pi Projects Book
Volume 5...
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ALMA observations of the debris disk around the young Solar Analog HD 107146
We present ALMA continuum observations at a wavelength of 1.25 mm of the debris disk surrounding the $\sim$ 100 Myr old solar analog HD 107146. The continuum emission extends from about 30 to 150 AU f...
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Fundamentals of Biomechanics
Equilibrium, Motion, and Deformation...
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Separated Fringe Packet Observations with the CHARA Array II: $\omega$ Andromeda, HD 178911, and {\x
When observed with optical long-baseline interferometers (OLBI), components of a binary star which are sufficiently separated produce their own interferometric fringe packets; these are referred to as...
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The Official Raspberry Pi Handbook 2021
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An M-dwarf star in the transition disk of Herbig HD 142527; Physical parameters and orbital elements
HD 142527A is one of the most studied Herbig Ae/Be stars with a transitional disk, as it has the largest imaged gap in any protoplanetary disk: the gas is cleared from 30 to 90 AU. The HD142527 system...
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Investigating transition state resonances in the time domain by means of Bohmian mechanics: The F+HD
In this work, we investigate the existence of transition state resonances on atom-diatom reactive collisions from a time-dependent perspective, stressing the role of quantum trajectories as a tool to ...
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