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Trans-Neptunian objects as natural probes to the unknown solar
Trans-Neptunian objects as natural probes to the unknown solar

... was an optimal candidate to be the source of SPCs, based on two main results. First, the inclination distribution of objects leaving the trans-Neptunian belt was dynamically preserved after entering into the inner solar system (modeled with i < 30 deg, roughly the same as that of the SPCs4). This ru ...
The white dwarf luminosity function
The white dwarf luminosity function

X-ray binaries in the Milky Way and other galaxies
X-ray binaries in the Milky Way and other galaxies

The Physical Origins of The Morphology
The Physical Origins of The Morphology

The Magnetic Field of the Earth
The Magnetic Field of the Earth

... (∇ · H = 0) and one must always consider a pair of opposite poles. Opposite poles attract and like poles repel each other. If the distance d between the poles is (infinitesimally) small → dipole. • Gravitational potential (or any potential due to a monopole) falls of as 1 over r, and the gravitation ...
Dimensionless Physical Quantities in Science and
Dimensionless Physical Quantities in Science and

USING STANDARD SYSTE - UW Madison Plasma Physics
USING STANDARD SYSTE - UW Madison Plasma Physics

Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies
Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies

... luminous galaxies form and initially evolve as disk galaxies at the center of isolated dark matter halos (DMH). Under this paradigm, as dark matter over-densities decouple from the large scale flow and collapse, the baryons of the ambient intergalactic medium bound to the potential well of the nasce ...
Physics of Neutron Star Crusts
Physics of Neutron Star Crusts

Physics of Neutron Star Crusts - Institut d`Astronomie et d
Physics of Neutron Star Crusts - Institut d`Astronomie et d

Instruction Manual/Experiments Guide
Instruction Manual/Experiments Guide

The effects of galaxy interactions on star formation
The effects of galaxy interactions on star formation

Titan at the edge: 1. Titan`s interaction with Saturn`s
Titan at the edge: 1. Titan`s interaction with Saturn`s

The Lupus clouds - European Southern Observatory
The Lupus clouds - European Southern Observatory

Stars and dust in the Galactic Center
Stars and dust in the Galactic Center

... Binned velocity dispersion used for Jeans modeling . . . . . . . Radial and tangential dispersions as function of the radius . . . Average radial velocities from our data and the literature . . . . Data and fits of the Jeans modeling . . . . . . . . . . . . . . . . Binwise median and maximum three-di ...
An axis-free overset grid in spherical polar coordinates for
An axis-free overset grid in spherical polar coordinates for

... spherical polar grid. It is straightforward to determine the corresponding interpolation coefficients. The mapping of vector quantities between the Yin and Yang grid patches requires an additional step. After interpolating the vector components they must be transformed according to the transformatio ...
1000-Solved-Problems-in-Classical-Physics-An-Exercise
1000-Solved-Problems-in-Classical-Physics-An-Exercise

Unfolding the Milky Way bulge - International Max Planck Research
Unfolding the Milky Way bulge - International Max Planck Research

Recent developments in gravitational collapse and spacetime
Recent developments in gravitational collapse and spacetime

A Review of the 0.1 Reconnection Rate Problem
A Review of the 0.1 Reconnection Rate Problem

Modeling the response of thin superconductors to applied magnetic
Modeling the response of thin superconductors to applied magnetic

Sample pages 1 PDF
Sample pages 1 PDF

Formation and evolution of giant molecular clouds in a barred spiral
Formation and evolution of giant molecular clouds in a barred spiral

The COMPLETE Survey of Outflows in Perseus
The COMPLETE Survey of Outflows in Perseus

Galaxies in the Universe: An Introduction, Second Edition
Galaxies in the Universe: An Introduction, Second Edition

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