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  2. Jeans instability - Wikipedia

    en.wikipedia.org/wiki/Jeans_instability

    The Jeans mass is named after the British physicist Sir James Jeans, who considered the process of gravitational collapse within a gaseous cloud. He was able to show that, under appropriate conditions, a cloud, or part of one, would become unstable and begin to collapse when it lacked sufficient gaseous pressure support to balance the force of gravity.

  3. List of hydrodynamic instabilities named after people - Wikipedia

    en.wikipedia.org/wiki/List_of_hydrodynamic...

    Faraday instability: Vibrating fluid surfaces: M. Faraday: Farley–Buneman instability: Plasma instability: Donald T. Farley and Oscar Buneman: Görtler instability: Stability of flow along a concave boundary layer: H. Görtler: Holmboe instability: Stratified shear flows: Jørgen Holmboe: Jeans instability: Stability of interstellar gas ...

  4. Plasma stability - Wikipedia

    en.wikipedia.org/wiki/Plasma_stability

    Firehose instability (a.k.a. hose instability), not to be confused with the similarly named Firehose instability in galactic dynamics; Fish instability, Free electron maser instability, Gyrotron instability, Helical (Helix) instability, Jeans instability, [23] [24] Magnetic buoyancy instability. Interchange instability (a.k.a. flute instability ...

  5. Toomre's stability criterion - Wikipedia

    en.wikipedia.org/wiki/Toomre's_Stability_Criterion

    The most basic gravitational stability analysis is the Jeans criteria, which addresses the balance between self-gravity and thermal pressure in a gas. In terms of the two above stability conditions, the system is stable if: i) thermal pressure balances the force of gravity, and ii) if the system is compressed slightly, the outward pressure ...

  6. Herbig Ae/Be star - Wikipedia

    en.wikipedia.org/wiki/Herbig_Ae/Be_star

    A Herbig Ae/Be star (HAeBe) is a pre-main-sequence star – a young (<10 Myr) star of spectral types A or B. These stars are still embedded in gas-dust envelopes and are sometimes accompanied by circumstellar disks. [1]

  7. Young stellar object - Wikipedia

    en.wikipedia.org/wiki/Young_stellar_object

    A star forms by accumulation of material that falls in to a protostar from a circumstellar disk or envelope. Material in the disk is cooler than the surface of the protostar, so it radiates at longer wavelengths of light producing excess infrared emission.

  8. These Are the Most Expensive Shoes Ever Sold at Auction

    www.aol.com/most-expensive-shoes-ever-sold...

    Sold for: $2.2 million. Worn by Jordan during Game 2 of the 1998 NBA Finals, these shoes witnessed the shooting guard score a whopping 37 points to lead the Bulls to victory on their path to a ...

  9. Category:Fluid dynamic instabilities - Wikipedia

    en.wikipedia.org/wiki/Category:Fluid_dynamic...

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