• Study Resource
  • Explore
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
Fluids - Duke Physics
Fluids - Duke Physics

... When the particles are on average far apart and only interact occasionally when they collide with each other, we have a gas. These situations define the three commonly occurring phases of matter. In the liquid and gas phases, the particles move about (flow) until the system takes the shape of the so ...
Pulsar slow glitches in a solid quark star model
Pulsar slow glitches in a solid quark star model

Simultaneous formation of solar system giant planets
Simultaneous formation of solar system giant planets

... architecture of the outer solar system (Morbidelli et al. 2009b). Remarkably, the Nice model does not say anything about how its own initial conditions could be achieved. More recently, Morbidelli & Crida (2007) – following the work of Masset & Snellgrove (2001) – showed that for certain parameters ...
ap physics b
ap physics b

CH15.AST1001.S15.EDS
CH15.AST1001.S15.EDS

... through stellar winds and planetary nebulae. © 2015 Pearson Education, Inc. ...
Momentum
Momentum

... using conservation of energy. mgh = ½ mv2 v = (2gh)1/2 = (2*9.8 m/s2*0.20 m) 1/2 = 2.0 m/s Calculate the brick’s momentum when it strikes the table. p = mv = (1.5 kg)(-2.0 m/s) = -3.0 kg m/s (down) The impulse necessary to stop the brick is the impulse necessary to change to momentum to zero. J = Dp ...
Gas Ejection from Spiral Galaxy Disks Jeremy Durelle
Gas Ejection from Spiral Galaxy Disks Jeremy Durelle

Stellar radii from long-baseline interferometry
Stellar radii from long-baseline interferometry

Evolution of a vortex in a magnetic field
Evolution of a vortex in a magnetic field

Looking for planets with SPHERE in planetary systems with double
Looking for planets with SPHERE in planetary systems with double

McConnell XGPolarimetry SSE
McConnell XGPolarimetry SSE

Phase-resolved high-resolution spectrophotometry of the eclipsing
Phase-resolved high-resolution spectrophotometry of the eclipsing

Electromagnetic braking: A simple quantitative model - if
Electromagnetic braking: A simple quantitative model - if

REPORTS Terahertz Magnetic Response from Artificial Materials
REPORTS Terahertz Magnetic Response from Artificial Materials

4 Newton`s Third Law
4 Newton`s Third Law

4 Newton`s Third Law
4 Newton`s Third Law

Chapter 15 THE MILKY WAY IN RELATION TO OTHER GALAXIES
Chapter 15 THE MILKY WAY IN RELATION TO OTHER GALAXIES

... size is difficult. Although studies on photographic plates are available from the earliest days of photometry (de Vaucouleurs (1957) observed the LMC very early on in his studies and determined the exponential nature of its disk), the prime method today is the use of CCD’s behind small telescopes (o ...
Electrostatics - PRADEEP KSHETRAPAL PHYSICS
Electrostatics - PRADEEP KSHETRAPAL PHYSICS

AAVSO: Epsilon Aurigae
AAVSO: Epsilon Aurigae

Evolution of filamentary molecular clouds in the presence of
Evolution of filamentary molecular clouds in the presence of

shock structures and momentum transfer in herbig
shock structures and momentum transfer in herbig

Work/Energy
Work/Energy

Magnetic Circuit Model and the Calculation of
Magnetic Circuit Model and the Calculation of

Halliday 9th chapters 10-11
Halliday 9th chapters 10-11

Magnetic field propagation in a two ion species planar plasma
Magnetic field propagation in a two ion species planar plasma

... the plasma ceases and the plasma pushing remains the dominant process. This is in contrast to cases shown in previous theoretical analyses, in which the penetration did not slow down due to the plasma pushing8 and was even enhanced by such a pushing.13 When there is more than one particle species, a ...
< 1 ... 28 29 30 31 32 33 34 35 36 ... 156 >

Accretion disk

  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report