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Magnetic Fields
Magnetic Fields

1. introduction
1. introduction

H 2 O, OH, SiO, NH 3 and CH 3 OH
H 2 O, OH, SiO, NH 3 and CH 3 OH

... Prestellar cores start off with similar masses. Their location within the molecular cloud determines the final mass of the star. High mass stars are formed in the cluster centres where the gas reservoir is denser. ...
Are turbulent spheres suitable initial conditions for star
Are turbulent spheres suitable initial conditions for star

The ultracompact nature of the black hole candidate X
The ultracompact nature of the black hole candidate X

The Trouble with Cosmological Magnetic Fields
The Trouble with Cosmological Magnetic Fields

... or even larger coherence scales Filaments: There are indications of magnetic fields in filaments with strengths up to B ∼ 10−8 – 10−7 Gauss and coherence scales over 1Mpc (Kronberg 2010). ...
Beams, Bursts, Bubbles, and Bullets: Relativistic Outflows in
Beams, Bursts, Bubbles, and Bullets: Relativistic Outflows in

... determined by this method, the observations are inconsistent with any compact object other than a black hole, and are thus the best evidence for the existence of black holes yet. Water Masers: Water masers have been detected from several AGNs, where they occur in the outer (molecular) part of the ac ...
SOLID STATE PHYSICS PART III Magnetic Properties of Solids
SOLID STATE PHYSICS PART III Magnetic Properties of Solids

Chapter 17 - Astronomy
Chapter 17 - Astronomy

Rotational Motion of Solid Objects
Rotational Motion of Solid Objects

CHEMICAL ABUNDANCE DISTRIBUTIONS OF GALACTIC HALOS
CHEMICAL ABUNDANCE DISTRIBUTIONS OF GALACTIC HALOS

Title The molecular envelope around the red supergiant VY CMa
Title The molecular envelope around the red supergiant VY CMa

Cold dark matter heats up
Cold dark matter heats up

Conservation Laws
Conservation Laws

... contributions coming from characteristics of the system such as motion of objects in it, heating of the objects, and the relative positions of objects that interact via forces. The total energy of a closed system always remains constant. Energy cannot be created or destroyed, but only transferred in ...
Physical Processes in the Interstellar Medium
Physical Processes in the Interstellar Medium

Chapter 7: Linear Momentum and Collisions
Chapter 7: Linear Momentum and Collisions

The physics of neutron stars
The physics of neutron stars

Classical Mechanics
Classical Mechanics

... for the position. Rewrite this equation in terms of the velocity and solve for ~v (t). Does your solution give the correct result for t → ∞? What is the physical meaning of this asymptotic value? Would you expect the time during which the ball rises to be longer or shorter than the time during which ...
Timing of the accreting millisecond pulsar IGR J17511-3057
Timing of the accreting millisecond pulsar IGR J17511-3057

Accreting millisecond X-ray pulsars, from accretion disk to magnetic
Accreting millisecond X-ray pulsars, from accretion disk to magnetic

... Moreover, neutron stars can rotate at spin periods near a millisecond, with surface velocities as high as several percent of the speed of light. Finally, neutron stars have magnetic fields which are among the strongest observed in the Universe: typical values range from B ∼ 108 Gauss for very old sy ...
Neutron stars: the densest state of condensed matter
Neutron stars: the densest state of condensed matter

Debris disks as signposts of terrestrial planet
Debris disks as signposts of terrestrial planet

Transparencies - Rencontres de Moriond
Transparencies - Rencontres de Moriond

...  3.8 and 4.8 µm IR source : on Sgr A* within 0.01"  Flux level fits very well expected spectrum  Flares and flashes from 1.6 to 3.8 µm : on Sgr A*  Simultaneous X and IR flare  Quiet emission : slightly extended and offset • Possible traces of a jet interaction with MIS ...
galaxy formation and evolution - Yale Astronomy
galaxy formation and evolution - Yale Astronomy

Investigating the Effects of Milky Way Globular Clusters
Investigating the Effects of Milky Way Globular Clusters

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